The galaxy presents an elliptical morphology, with a smooth light distribution. It displays a noticeable central bulge that transitions gradually into a fainter, more diffuse outer region. The color profile suggests a centrally concentrated, older stellar population dominating the core, indicated by the yellowish hue. The outer regions exhibit a bluer tint, suggestive of some ongoing, albeit low-level, star formation activity. There's a slight indication of a minor tidal disturbance, or perhaps a past interaction event, evidenced by a subtle asymmetry in the outer halo. There does not seem to be any evidence of recent major mergers, or strong star formation events. The galaxy's overall appearance is that of a relatively quiescent system undergoing slow evolution.
