The galaxy presents as a relatively compact, elliptical structure with a flattened profile. The core region exhibits a smooth, diffuse appearance, characterized by a dominant concentration of light. The luminosity appears to decrease gradually from the core towards the outer edges. Some subtle, patchy variations in color suggest areas of potential star formation or dust obscuration within the galaxy, although it is mostly homogenous. The overall color index indicates a population of older stars, potentially an early-type galaxy. There is a faint disk-like structure. There is no evidence of significant spiral arm structures. The image suggests no major mergers or tidal disturbances.
