The galaxy appears to be an elliptical system, although a weak disk structure cannot be ruled out due to the limitations of image resolution. The core of the galaxy is bright and centrally concentrated, indicating a high density of stars and potentially a supermassive black hole at the center. The galaxy exhibits a mostly smooth, symmetric profile with a round morphology, suggesting it is relatively relaxed and has not undergone a major merger recently. There is some asymmetry visible in the outer regions, with some areas appearing slightly disturbed or diffuse, which could be indicative of a minor interaction with a smaller galaxy or the remnant of a past merger event. A slight color gradient is present, with the core appearing bluer than the outskirts, possibly signifying ongoing star formation in the central region.