The galaxy presents as a relatively symmetrical, elliptical-like structure. It exhibits a smooth, centrally concentrated luminosity profile, with a bright core that gradually fades into the outer regions. There is a slight elongation, but no obvious bar structure or spiral arms are discernible in this image. The galaxy appears primarily smooth and well-defined. There is no noticeable dust lane bisecting the galaxy. The overall color suggests a slightly older stellar population. No evidence of tidal tails or significant morphological disturbance is apparent, indicating it is likely not undergoing a major merger event. Based on the observed characteristics, it is probable that the galaxy is an early-type galaxy, specifically an elliptical galaxy of moderate size and mass with a low star formation rate.
