The galaxy presents as a smooth, elliptical-shaped object with a central bulge that appears more luminous than the surrounding galactic disk. The color profile suggests a population of older stars. There is some evidence of a faint, diffuse disk component surrounding the central bulge. The galaxy does not display any obvious spiral arm structure. It appears relatively undisturbed, without any strong signs of tidal interactions or recent major mergers. The overall color indices suggest intermediate star formation rate, with a moderately high mass. The object exhibits an elongated shape, potentially indicative of a prolate spheroid structure, or possibly, a galaxy undergoing a minor tidal interaction.
