The galaxy presents as a moderately bright, elliptical-shaped structure. Its light distribution appears relatively smooth and centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is a hint of a possible tidal feature or minor disturbance on the outer edge, suggesting a past interaction or ongoing accretion event, however, the overall morphology is consistent with an early-type galaxy possessing a large stellar mass. The color profile indicates a higher concentration of older stellar populations, leading to an orangish appearance, consistent with a low star formation rate. This object lacks prominent spiral arms or any other distinctive features typically associated with actively star-forming galaxies.
