The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile is concentrated towards the center, displaying a bright, yellowish core. The outer regions exhibit a gradual decrease in surface brightness, fading into the background. The overall color suggests a population dominated by older stars, indicative of an evolved stellar population. There is little to no evidence of prominent spiral arms or dust lanes, supporting a classification towards early-type galaxies. Subtle asymmetry may suggest minor past interaction, however, no substantial merging or tidal features are apparent. The galaxy's apparent roundness and lack of distinct features suggest a relaxed morphology.
