This galaxy appears as a moderately luminous, elliptical or lenticular system. It exhibits a smooth, concentrated central bulge with a gradual decline in surface brightness towards the edges. There is a slight elongation, suggesting it is not perfectly spherical, but rather somewhat flattened. No distinct spiral arm structures are visible in the image. The color profile indicates a predominantly older stellar population, with a yellowish-white hue. There are no significant signs of ongoing major merger activity or tidal disturbances that are immediately apparent. It seems the galaxy is a relatively undisturbed system.
