The galaxy appears as a somewhat compact, elliptical-shaped structure. Its color profile indicates a redder hue, suggesting an older stellar population. The light distribution is smooth and concentrated towards the center, lacking significant spiral arm features or distinct substructures. There may be a very slight asymmetry or faint tidal feature hinting at a past interaction, but it is not a disturbed image. The core appears slightly brighter than the outer regions, indicating a possible concentration of older stars or a weak active galactic nucleus.
