The galaxy presents a generally smooth, elliptical morphology. There is a concentrated, bright central bulge that appears slightly yellow. The galaxy shows a gradual decrease in luminosity from the center outwards, with a faint, diffuse halo extending beyond the central region. There are no discernible spiral arms or bar structures. The overall shape appears fairly round, with no major distortions or signs of an ongoing merger event. Minor disturbances cannot be ruled out due to the resolution. Based on the color gradient, there may be some evidence of recent or ongoing star formation within the galaxy, though it appears to be a relatively quiescent system.
