The galaxy presents as an elliptical morphology, appearing largely smooth with a high degree of central concentration of light. There is evidence of a faint, diffuse halo extending beyond the brighter central region. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region, hinting at evolved stars. There is a hint of asymmetry and minor disturbances in its outer regions. The general shape appears more in-between than perfectly round or cigar-shaped. There is no apparent indication of a major merger event, though minor disturbances cannot be ruled out. Star formation appears to be occurring at a moderate rate. Overall, the galaxy exhibits characteristics of a massive, relatively evolved system, possibly undergoing minor evolutionary changes.
