The galaxy appears to be an elliptical galaxy. It exhibits a generally smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The galaxy presents a concentrated central bulge region that transitions into a more diffuse halo. The color profile suggests a population of older stars. It is approximately spherical in shape. There is no evidence of active galactic nuclei activity. This galaxy appears to be a relatively massive and passive system. Faint tidal features suggest a previous minor merger, but there are no signs of an ongoing major interaction.