The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a bright, yellowish-white luminosity, indicating a population of older stars. The outer regions of the galaxy fade into a less defined halo. There is a lack of distinct spiral arm structures. The overall roundness suggests a system that is relatively relaxed, without significant signs of recent mergers or major disturbances. Faint, diffuse bluer colors are intermixed with a redder halo suggesting star formation. There are no prominent dust lanes or distinct features indicating ongoing major starburst activity. It exhibits an old stellar population and minimal signs of active star formation.
