The galaxy presents an elongated, cigar-like morphology. A bright, concentrated central bulge is apparent, exhibiting a yellowish hue. Extending outwards from the bulge, the galaxy appears to have a faint, disk-like structure with hints of bluer regions, suggestive of areas with recent or ongoing star formation. There is no evidence of a distinct spiral arm structure or a prominent bar feature. The overall appearance suggests a galaxy transitioning from a more active, star-forming state to a more quiescent one. The lack of significant dust lanes or pronounced features implies that we are observing a relatively evolved system. There is slight asymmetry, potentially due to minor tidal interactions or internal dynamics.
