The galaxy exhibits a roughly elliptical morphology, with a distinct, though somewhat irregular, disk structure. There is a clear central bulge which appears bright and somewhat diffuse. 

Moving outwards from the bulge, the disk shows evidence of some structure, perhaps indicative of spiral arms or tidal features. The color gradients suggest differing stellar populations or dust distributions within the disk. The galaxy’s color is notably bluer in the outer regions of the disk. There appears to be an interaction or possible merging event occurring, seen in the warped and disturbed appearance of the disk. The overall structure is slightly disturbed or asymmetrical, possibly caused by the interaction.
