The galaxy appears to be elliptical in shape, with a smooth, centrally concentrated light profile. The core exhibits a bright yellowish hue, suggesting an older stellar population. There is a gradual decrease in surface brightness towards the outer regions, with a faint, diffuse halo extending outwards. The galaxy's overall color gradient implies a potential lack of significant ongoing star formation. No distinct spiral arms or dust lanes are discernible. The overall morphology is consistent with an early-type galaxy. A slight elongation is observed. There is no evidence of tidal tails or strong interactions.
