The galaxy presents as a largely featureless, elliptical-like structure with a smooth light distribution. It exhibits a concentrated central region, likely indicative of a galactic bulge. The overall color appears slightly redder compared to the surrounding field, implying a population of older stars and reduced ongoing star formation. There is little evidence of spiral arms, a disk-like structure, or significant dust lanes. The galaxy's shape is roughly circular in projection. No signs of strong tidal interactions or merging activity are readily apparent. Faint, diffuse light extends outwards from the core, suggesting a galactic halo. The color and morphology, along with estimated size and brightness, suggest it is a relatively massive system.