The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge is prominent and exhibits a concentrated brightness, suggesting a high density of stars, likely older populations. The overall color gradient shifts from a more yellowish-red core region to a bluer halo, potentially indicating a radial distribution in stellar population ages, with older stars concentrated in the center and younger stars residing in the outer regions. Although a disk structure is not immediately obvious, there appears to be some flattening, suggesting it is likely an elliptical galaxy but not perfectly spherical. There are minor disturbances in the morphology but overall the galaxy appears as a system that is undergoing minimal merging activity. Star formation is not prominent but is likely occurring at a low rate.
