The galaxy presents a complex morphology, appearing as a spiral galaxy with a relatively prominent bulge. The bulge exhibits a bright, concentrated core and a yellowish hue, which may suggest an older stellar population. Faint spiral arms are observed extending outwards from the central bulge, displaying a slightly blue color. This may indicate regions of more recent or ongoing star formation. There are noticeable asymmetries and disturbances in the arms, especially with clumpy knots of star formation in both spiral arms. Patches of reddish dust lanes are also visible within the arms, particularly on the lower spiral arm, which may be obscuring background starlight. The galaxy appears to be undergoing some degree of interaction, possibly through tidal forces and mergers. There is evidence of a central bar structure, extending slightly vertically through the galaxy, but it is not very bright. The outer edges of the galaxy are very faint and do not have a clear, distinct edge. The center of this galaxy appears to have many merging features occurring. Overall, this galaxy's morphology shows disk features and distortions potentially due to interactions with other galaxies or internal processes.