The galaxy presents as a relatively smooth, rounded structure with a concentrated central bulge exhibiting a yellow-orange hue. This color suggests an older stellar population dominating the core, implying reduced star formation activity in that region. A fainter, slightly bluer, and smaller companion object is visible in close proximity, which could be a dwarf galaxy or a region of active star formation within the primary galaxy or a foreground object. The primary galaxy exhibits a subtle disk-like structure, though it is not sharply defined. There is no evident presence of strong spiral arms. Overall, the galaxy appears to be a relatively evolved system, possibly an elliptical or lenticular type, with the suggestion of a potential interaction or merging event in progress.
