The galaxy presents as a fairly compact and luminous object. Its morphology is generally smooth, appearing elliptical or spheroidal in shape, with no readily discernible spiral arms or disk-like features. There is a concentration of light towards the center of the galaxy, indicating the likely presence of a galactic nucleus. The radial light profile appears to decrease smoothly from the center outwards. The color gradient suggests a population of older stars and/or significant dust obscuration. There is no evidence of ongoing major mergers or tidal disturbances. The galaxy is not perfectly circular but deviates slightly, appearing somewhat elongated. Overall, this galaxy appears to be a relatively evolved system, likely a massive elliptical galaxy.
