The galaxy presents a somewhat elongated, cigar-shaped morphology. A significant portion of the galaxy appears smooth in texture, although there are hints of disk-like features. The light distribution is not uniform, with a noticeable concentration toward one end, potentially indicating the presence of a bulge or core. There's a distinct color gradient across the galaxy, transitioning from bluer hues at one extremity to redder, yellower tones at the opposite end. This color variation might indicate varying stellar populations, with younger, bluer stars concentrated in one region and older, redder stars in another. Overall, the galaxy exhibits a complex structure possibly suggestive of a galaxy undergoing tidal disruption or merger.
