This galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. The core is a bright, almost uniform white, while the outer regions show hints of subtle color variations, possibly indicating differences in stellar populations. There are no apparent spiral arms or distinct features typically associated with disk galaxies. The galaxy appears largely undisturbed, without any obvious signs of major mergers or tidal interactions, though minor disturbances may not be visible at this resolution. The overall morphology suggests a system dominated by older stellar populations, possibly with a moderate rate of on-going star formation.
