The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a centrally concentrated bright core with a diffuse, less luminous halo extending outwards. The overall color profile suggests a population of older stars, contributing to the galaxy's slightly reddish hue. There is a faint hint of a possible disk component, or at least a flattening, but it's subtle. Based on its morphology, it may be undergoing minor gravitational interaction with a neighboring object, though no significant tidal features are readily apparent. The galaxy's central bulge appears to dominate its overall light profile.
