The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, indicating a population of older stars. This central bulge smoothly transitions into a fainter, more diffuse halo. There are no readily apparent spiral arm structures or prominent dust lanes. The overall shape of the galaxy appears to be more elongated than circular, suggesting a classification somewhere between elliptical and lenticular. Faint indications of minor tidal disturbances are present, possibly indicating previous or ongoing interactions with other galaxies, although a definitive merger event is not obvious. The size of the object appears relatively compact.
