The galaxy appears as a relatively compact object with a diffuse halo. It exhibits a somewhat irregular morphology, and there is a slight indication of a disk-like structure, though it is not well-defined. Some asymmetry is evident in the light distribution. A subtle feature, potentially a minor disturbance or tidal tail, is faintly visible on one side of the galaxy, suggesting a possible interaction or past merger event. The galaxy's color appears reddish, potentially indicating an older stellar population or significant dust obscuration. The overall light distribution suggests a moderate concentration towards the center, though not exhibiting a distinct bulge.
