The galaxy presents a primarily smooth, elliptical morphology, appearing largely featureless. It exhibits a concentrated central bulge that gradually fades into a more diffuse halo. The color gradient suggests a stellar population dominated by older, redder stars, concentrated towards the center. There is a subtle hint of a flattened disk-like structure, although this is not a dominant feature. No significant signs of ongoing major mergers or tidal disturbances are readily apparent.
