The galaxy presents a largely smooth and rounded appearance, with a concentrated central bulge exhibiting a yellowish hue. This suggests a population of older stars dominating the core. The outer regions of the galaxy show a faint, more diffuse structure, possibly indicating a weak or unresolved spiral arm structure. The overall color is relatively uniform, although there is a subtle shift towards redder tones in the central region compared to the outer areas. This could indicate a radial color gradient, with older stellar populations more concentrated towards the center and relatively less ongoing star formation activity. There is a relatively small object near the galaxy that seems to be interacting with it, possibly a dwarf galaxy in the process of merging or a tidal stream, though without further data it's not possible to make any conclusions about it.
