The object presents as a relatively small, elliptical galaxy. The central region exhibits a bright, concentrated core, suggesting a possible active galactic nucleus or a dense stellar population. A fainter, somewhat diffuse halo surrounds the central core, appearing asymmetrical and elongated along a single axis. This elongation may indicate a possible ongoing merger or tidal interaction. The color gradient indicates varying stellar populations. The central core appears bluer, potentially indicative of younger stars. The outer regions become redder, suggesting older stellar populations. Overall, the galaxy exhibits a smooth appearance, but there are subtle features that warrant further investigation.
