The galaxy presents as a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the light profile. Moving outward from the center, there is a gradual decline in surface brightness, with the outer regions appearing more diffuse. The galaxy exhibits a subtle color gradient, with the core appearing somewhat more yellow or gold compared to the bluish-white hues in the extended halo. There is little evidence of spiral arm structure or prominent dust lanes. The overall appearance suggests a relatively evolved system, potentially an early-type galaxy with minimal ongoing star formation. Faint disturbances can be noted on the outskirts that suggest that the system may be experiencing or have experienced a minor merger.
