This galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated brightness profile, with light intensity gradually decreasing outwards from the core. The galaxy is generally round in shape, displaying no obvious signs of a disk-like structure or spiral arms. There are hints of subtle color variations, with a slightly bluer hue in the outer regions compared to the yellower core, possibly indicating some ongoing, though limited, star formation activity. No clear indications of major mergers or significant tidal disturbances are observed. Overall, this galaxy presents as a well-formed, evolved system.
