The galaxy exhibits a largely smooth morphology, appearing elliptical in shape. It displays a concentrated central bulge that transitions gradually into a diffuse halo. The overall color appears to be a reddish-gold, suggesting an older stellar population and potentially a lack of ongoing, significant star formation. No distinct spiral arms or dust lanes are discernible. There is a subtle asymmetry, possibly indicative of a minor interaction or past disturbance, though it's not a pronounced merging event. The galaxy appears to be relatively isolated, without any clear evidence of a close companion galaxy readily visible.