The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness. Its shape is more in-between, not quite perfectly round and not strongly elongated. There is no evident disk structure, and the galaxy appears largely undisturbed, showing no signs of recent major mergers or significant tidal interactions.

The color profile of the galaxy tends towards the redder end of the spectrum. It presents a concentrated central bulge surrounded by a more diffuse halo. No distinct spiral arm structures or prominent dust lanes are observed. Given the red color and smooth morphology, the galaxy likely hosts a population of older stars and a comparatively low star formation rate. It is a massive galaxy.
