The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, with a high degree of circular symmetry. The central region exhibits a bright, concentrated core, suggesting a substantial stellar population or potentially an active galactic nucleus. The galaxy displays a gradual decrease in surface brightness moving from the center outwards, with no distinct spiral arm features or prominent dust lanes visible. The color appears generally redder, indicating an older stellar population with diminished ongoing star formation. There is no evidence of recent major merger events or significant tidal disturbances in its immediate vicinity. The overall impression is that of a well-evolved, relatively quiescent galaxy.
