The galaxy presents a mostly smooth, elliptical morphology. It appears relatively isolated, with no immediately obvious signs of major interaction or tidal features. The light distribution indicates a concentrated central bulge, which fades gradually outward. The color gradients suggest that the central region hosts an older stellar population, while the outer regions may have more recent star formation, though at a very low rate. The galaxy exhibits a slight elongation, with an apparent inclination to our line of sight. The overall appearance suggests a evolved system.
