The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse halo extending outwards. There is a hint of a disk-like structure or perhaps faint spiral arms, though these features are not prominent and might represent a minor disturbance within the galaxy's overall smooth structure. The galaxy appears relatively isolated with no signs of significant tidal interactions or ongoing merger events with other galaxies. The color gradient indicates a population of older stars dominating the galaxy's stellar content, with a subtle presence of bluer components suggesting regions of recent, albeit suppressed, star formation. The overall light distribution suggests an evolved system approaching a quiescent state. The angular size is relatively small, consistent with a galaxy at a moderate cosmological distance, and the galaxy is bright enough to have been detected in multiple color bands, suggesting high luminosity.
