The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a high concentration of older stars. The galaxy has a golden hue overall, suggesting an older stellar population, with a possible red shift. There is a hint of tidal disturbance suggesting that the galaxy could be undergoing a merger. A smaller, less defined secondary body appears close to the primary structure, possibly indicating an ongoing interaction or recent merger event. The smooth nature of the galaxy suggests it has either completed its merger or is currently in the late stages of a major merger event. The galaxy exhibits a low star formation rate.
