The object presents as a relatively compact galaxy, exhibiting a smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual falloff towards the outer regions. There is little evidence of spiral arms or a defined disk structure. The galaxy's color is slightly yellow-reddish, suggesting a population of older stars with subdued star formation. There is no indication of significant dust lanes or prominent HII regions. No major mergers or tidal disturbances are immediately apparent, though minor interactions or past mergers cannot be ruled out. The galaxy appears to be relatively isolated.
