The galaxy presents a largely smooth, elliptical morphology. It appears highly rounded, exhibiting a near-perfect circular symmetry in its overall shape. There is no discernible disk structure or spiral arm features visible at this resolution. The galaxy’s light distribution is centrally concentrated, with a gradual decrease in surface brightness moving outward from the core. The core region exhibits a yellowish hue suggesting an older stellar population. There is a subtle color gradient, where the outer regions appear slightly redder, hinting at variations in stellar population or dust content. The overall color indices point to a red sequence galaxy. There are no obvious signs of ongoing mergers or major tidal disturbances, although subtle asymmetries or minor disturbances cannot be entirely ruled out at this image resolution. This galaxy's stellar mass is very high. The star formation rate appears to be low. The galaxy likely falls under the classification of a passive, early-type galaxy.
