The galaxy presents as a smooth, elliptical-like structure with a centrally concentrated light profile. There is a distinct core region exhibiting a bright, yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy display a gradual decrease in luminosity, appearing more diffuse and somewhat flattened. A very faint disk is possibly observed around the central region. No distinct spiral arm structures are discernible. There is some subtle irregularity in the outer regions of the galaxy, which could indicate a minor disturbance or interaction. Overall, the galaxy is likely a relatively massive system, showing moderate star formation.
