The object appears to be a relatively smooth, centrally concentrated galaxy. It exhibits a roughly elliptical morphology, tending towards a circular shape. There is a suggestion of some internal structure, possibly related to a faint disk or spiral arms, but this is subtle. The galaxy displays a color gradient, with a yellowish-white core transitioning to a greenish-blue hue in the outer regions. The smooth appearance suggests that the galaxy is relatively evolved and likely contains a significant population of older stars. There does not appear to be any evidence of ongoing major merger activity or significant tidal disturbances in the immediate vicinity.
