The galaxy presents as an elliptical morphology, exhibiting a concentrated central bulge that graduates into a more diffuse halo. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central regions. Fainter, bluer tinges are visible in the outer regions indicating a slightly younger stellar population. There are hints of a disk-like structure, but there are no readily apparent spiral arms. There is no obvious signs of active star formation. It does not appear to be undergoing a major merging event, and the general shape appears relatively undisturbed.
