The galaxy presents as a singular, concentrated object with a generally smooth morphology. It exhibits a spheroidal shape, appearing largely round. There is no clear evidence of spiral arm structures or a prominent disk. The light profile appears centrally concentrated with no indication of a distinct core or ring-like feature. There are no obvious signs of ongoing major mergers or significant tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed, well-formed system, likely an elliptical galaxy. The color suggests a population of older stars, potentially with limited ongoing star formation.
