The galaxy presents an elliptical morphology, elongated with an approximate axis ratio of 3:5. It exhibits a smooth, centrally concentrated light profile. Color gradients suggest an older stellar population, with a redder core transitioning to slightly bluer, fainter outer regions. There is a faint distortion in the galaxy's halo on the far right. This suggests a possible minor gravitational interaction with another small object that is barely visible. No prominent dust lanes or spiral arm structures are apparent.
