The galaxy appears to be a relatively smooth, centrally concentrated system. The light profile suggests a bulge-dominated morphology, with a gradual decrease in luminosity extending outwards. The galaxy exhibits a slightly elliptical shape, but is close to being circular. There is no apparent spiral arm structure or evidence of a prominent disk. The color appears yellowish-white, potentially indicating a population of older stars and a relatively low rate of ongoing star formation. There are no obvious signs of significant tidal disturbances or mergers affecting the overall structure of the galaxy.
