The observed galaxy presents as an edge-on spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, rounded morphology, concentrated in the center of the galaxy. A disk structure is distinctly visible, extending outwards from the bulge in a linear fashion. The disk shows a relatively smooth texture, with no apparent distinct spiral arm features visible at this resolution. Dust lanes are likely obscuring detailed features within the disk. There is no indication of a major merger event; however, some minor disturbances can't be ruled out given the limitations of the image quality. The color profile appears redshifted, with bluer light towards the outer edges of the disk and redder light concentrated within the bulge. This color gradient could suggest active star formation regions in the disk and an older stellar population in the bulge. The galaxy overall appears relatively isolated with no obvious nearby interacting galaxies.
