The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, characterized by a yellowish hue, indicative of an older stellar population. Fainter, diffuse extensions appear to emanate from the core, gradually fading into the background sky. These outer regions appear to have slightly bluer tones than the center. There is no clear evidence of spiral arms or a prominent disk component. The overall morphology suggests a system that has largely completed the process of hierarchical galaxy formation. No significant signs of tidal interactions or recent mergers are apparent in the immediate vicinity.
