The galaxy presents a smooth, elongated morphology, indicative of an elliptical or lenticular type. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards its outer regions. The overall color appears slightly reddish, suggesting an older stellar population and a relatively low rate of current star formation. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy is somewhat cigar-shaped, and it seems to be an isolated galaxy, showing no signs of major interaction or ongoing merger activity.
