The galaxy presents an elliptical morphology, with a predominantly smooth light distribution. The overall color is a warm, reddish hue, with a brighter, more compact and bluer core region, which suggests a younger stellar population or the presence of an active galactic nucleus (AGN). A faint, elongated feature extends outward from the central region, potentially indicating a tidal interaction, a minor merger, or a distorted structure. The primary body of the galaxy exhibits a relatively high degree of symmetry. The color gradient indicates a radial change in stellar populations or dust content.
