The galaxy presents a generally smooth and elliptical morphology, with a centrally concentrated luminosity profile. The object appears largely spheroidal, with a high degree of roundness and a lack of discernible spiral arm structure. The color gradient suggests a population of older stars dominating the core, which shifts toward bluer hues within its surrounding regions. There's a subtle hint of some low level disturbances in the outer halo, possibly indicative of past minor interactions. The overall appearance is consistent with a relatively quiescent galaxy, possibly undergoing only moderate levels of star formation.
