The galaxy presents as a relatively smooth, single object with a discernible central concentration. Its overall shape is largely round, exhibiting minimal deviation from circular symmetry. There is a slight elongation or distortion, potentially indicating a minor disturbance or interaction with another object.

The galaxy displays a color gradient, with the central region appearing more yellowish-orange and the outer regions exhibiting a slightly bluer hue. This suggests a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outer regions. There does not appear to be strong evidence of significant spiral arm structure or prominent dust lanes. A small concentration appears to be pulling away, as if being disrupted by the main body. This is likely a smaller dwarf galaxy.
