The observed galaxy presents an elliptical morphology, appearing generally smooth in structure with a concentrated central bulge. Its overall color index appears redder, suggesting an older stellar population. The primary color is yellow-white. There appears to be a slight asymmetry in the outer regions, which could be the result of minor gravitational interactions or internal dynamics. No clear spiral arms or dust lanes are visible. The galaxy's shape is somewhat elongated, with the major axis appearing to be a few times larger than the minor axis. There are no obvious signs of a recent major merger, although subtle disturbances cannot be ruled out without further analysis.
