The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution is concentrated towards the center, showing a bright, unresolved core. There is a noticeable radial decrease in surface brightness outwards from the core, with a faint, diffuse halo extending beyond the central region. No distinct spiral arms or prominent features are discernible. The galaxy appears largely symmetrical and undisturbed. The color profile suggests a population of older stars, contributing to the observed redder hue. There are no signs of ongoing major mergers or tidal disruptions, suggesting a relaxed and evolved system.
