The galaxy presents as an elliptical morphology, elongated in shape. Its core appears concentrated and exhibits a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy display a gradual decrease in luminosity, fading into the background sky. There is little to no evidence of spiral arm structure or prominent dust lanes. The galaxy exhibits a relatively smooth texture, lacking obvious signs of recent merger events or significant star formation activity. A slight asymmetry is present.
