The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a high degree of central concentration with a bright core region, diminishing in intensity outwards. There is no visible evidence of spiral arms, bar features, or significant dust lanes. The galaxy appears to be quite rounded in shape. There is no obvious indication of any major ongoing merging activity or tidal distortions. The overall color of the galaxy appears to be relatively red, likely indicative of an older stellar population. While there may be some minor disturbances, the galaxy does not appear to be actively undergoing a major interaction with another galaxy.
