The galaxy presents as a relatively bright, elliptical-like structure with a concentrated central bulge. The core region is characterized by a yellowish-white hue, suggesting an older stellar population. Extending outwards from the core, the galactic halo appears less luminous and exhibits a more diffuse, asymmetric distribution of light. There seems to be a slight tidal tail or stream extending from the galaxy. The overall morphology hints at a possible interaction or past merger event, with signs of disturbance in the outer regions. There are no clearly defined spiral arm structures visible. The galaxy appears tilted with an approximate axial ratio of ~0.75.
