The galaxy presents as a relatively smooth and centrally concentrated object. There is a discernible elliptical shape to the overall structure. The core region appears quite luminous, suggesting a high density of stars or an active galactic nucleus. The light distribution shows a gradual decrease in brightness from the center outwards. The color profile indicates a predominantly older stellar population as the galaxy appears redder in the outer regions compared to the core. There is a faint hint of blue around the central bulge suggesting a small presence of younger stars or ongoing star formation. It shows no clear signs of spiral arms or a disk structure. The overall morphology points towards an early-type galaxy, possibly an elliptical. There are no apparent major disturbances such as tidal tails or strong asymmetries, suggesting that this galaxy has not undergone a major merger event recently. The outskirts of the galaxy blend smoothly into the background, indicating a lack of prominent features at the observed wavelengths.