The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central region, likely a galactic nucleus, which appears bright and yellowish. A diffuse halo surrounds the central region, displaying a bluer hue, which potentially indicates the presence of younger stellar populations or ongoing star formation. The galaxy's shape is largely rounded, with only minor deviations from perfect circularity. There is a slight indication of a possible disturbance in the galaxy's outer regions. Overall, the galaxy appears to be relatively isolated, with no signs of a major merger event.
