The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is no discernible spiral structure or bar. The light distribution appears relatively uniform, lacking distinct features such as prominent dust lanes or star-forming regions. A slight color gradient is observed, trending towards a redder hue in the central region, suggestive of an older stellar population. The outer regions exhibit a bluer tint, possibly indicating younger stars, or low-level ongoing star formation. The overall smoothness and roundness indicate that the galaxy has likely undergone significant dynamical relaxation. There is no evidence of tidal tails, ongoing mergers, or significant disturbances, implying that it is in a relatively quiescent state. The galaxy is compact, possessing a relatively high surface brightness.
