The galaxy appears as a centrally concentrated, relatively smooth object with a slightly elliptical morphology. The color profile indicates a dominant yellowish-orange hue, suggesting an older stellar population. There is a lack of discernible spiral arm structure or prominent dust lanes. The galaxy exhibits a high degree of central light concentration, with a gradual decrease in surface brightness towards its outer regions. There are no indications of tidal tails or other obvious signs of recent major merger activity. Minor asymmetry may be present in the outer regions. Overall, the galaxy is consistent with a likely early-type galaxy, possibly an elliptical or lenticular galaxy.
