The galaxy presents as a moderately bright, elliptical form with a clearly defined core. The central region exhibits a high surface brightness, appearing almost uniformly illuminated. A discernible, though not sharply delineated, disk-like structure surrounds the central bulge. This disk displays a bluer hue, potentially indicative of ongoing star formation. The overall color profile suggests a population of both older, redder stars concentrated towards the center and a younger, bluer population in the outer regions. There is faint structural irregularity, possibly indicative of a minor disturbance or interaction. Overall, the galaxy's morphology suggests a later-type spiral galaxy with a significant spheroidal component.
