The galaxy appears to be a relatively smooth elliptical type. It exhibits a bright, concentrated core that graduates outward into a more diffuse halo. The shape is somewhat elongated, leaning towards a cigar-like form, but still maintains a mostly rounded appearance. There is no discernible disk structure or spiral arms. The overall color profile shows a subtle gradient, shifting from a bluer center to slightly redder outer regions, indicating a potential presence of younger stars in the core region, contrasted with older stellar populations further out. There might be some minor disturbance in the galaxy's morphology; however, it primarily showcases a singular structure with no strong indications of merging activity.
