The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, appearing brightest towards the core and gradually diminishing outwards. The core region is characterized by a yellowish-white hue, suggesting an older stellar population. The galaxy lacks any distinct spiral arm features or prominent dust lanes. The overall shape is approximately round, with a smooth transition from the central bulge to the outer regions, the galaxy does not have any other galactic bodies interacting with it. There might be slight disturbances of it's shape, but the disturbance is minor and has not affected the galaxies overal structure. The galaxy appears to be relatively isolated, without any signs of significant tidal interactions or ongoing mergers. It is most likely currently undergoing moderate star formation.