The galaxy appears as a relatively smooth, elliptical structure. Its light profile is centrally concentrated, with a gradual decrease in surface brightness towards the outer regions. The galaxy's shape is somewhat elongated, not perfectly spherical, leaning towards an in-between shape. There is no obvious disk structure or spiral arms visible. The galaxy exhibits a yellow-red hue suggesting a population of older stars and a low rate of ongoing star formation. There is no strong evidence of tidal features, major mergers, or significant dust lanes within the galaxy's structure. Possible minor disturbances are slightly hinted at but not clearly visible.
