The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color profile indicates a dominant population of older stars, with a yellowish-white hue. There is no discernible spiral arm structure or significant dust lane features visible. The galaxy's shape appears mostly rounded but it is not perfectly spherical, instead falling somewhere between round and elliptical. There's no evidence of major disturbances such as tidal tails or obvious signs of a recent or ongoing merger. It is more likely that the galaxy is undergoing little to no star formation activity. The stellar mass of this galaxy appears large.
