The galaxy presents a primarily elliptical morphology, displaying a smooth, centrally concentrated bulge. There are hints of a faint, extended disk component, although the image resolution makes it difficult to definitively characterize its structure. The galaxy exhibits a color gradient, with the central regions appearing more yellow-orange, suggesting a higher concentration of older stellar populations. The outer regions show a slightly bluer hue, potentially indicative of younger stars or ongoing star formation. There are some minor disturbances possibly from a minor merger event. Overall, the galaxy appears to be a massive system with a considerable stellar mass, exhibiting moderate star formation activity.
