The galaxy presents as a somewhat diffuse, elliptical object. It exhibits a smooth morphology, lacking prominent spiral arms or distinct features typically associated with disk galaxies. There is evidence for a slight disturbance or interaction with a smaller companion galaxy, but is likely not undergoing a major merging event. The galaxy's color index suggests a population of older stars, resulting in a redder appearance. Although some star formation is present, it does so only at a low rate. The overall shape appears close to circular in the image.
