The galaxy exhibits a generally elliptical morphology. The core is intensely bright, suggesting a high concentration of stars. The color of the core is notably redder compared to the outer regions. Moving outward from the core, the galaxy transitions to a more diffuse, bluer halo. The overall structure appears somewhat disturbed, possibly indicating an interaction or merger event in its past. There are hints of tidal features or asymmetries in the outer regions, but they are not pronounced. The object does not appear to be a pure elliptical, showing some characteristics of a disk galaxy.