This galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a relatively high degree of symmetry. The light distribution is centrally peaked, indicating a high concentration of stars in the core region. The galaxy displays a gradual decrease in surface brightness from the center outwards, with no apparent spiral arm structures or prominent dust lanes.

Color gradients are subtle, but present. The core appears to exhibit a slightly more yellow/orange hue compared to the outer regions, suggesting the presence of an older stellar population within the central bulge. The outer regions exhibit a more bluish hue, indicative of possible ongoing star formation, albeit at a low rate. There is no evidence of strong tidal features or morphological distortions, suggesting that it is not currently undergoing a major merger event. Subtle disturbances may be present.
