The galaxy presents as a relatively smooth, elliptical form. It exhibits a concentrated central bulge, with the light intensity decreasing gradually towards the outer edges. The color profile suggests a primarily older stellar population, with a yellowish hue dominating the overall appearance. There appears to be some subtle hints of bluer regions, potentially indicative of recent or ongoing star formation, though these are minimal. The galaxy's shape is more elongated than spherical, appearing as a flattened ellipsoid. There's no clear evidence of a disk component or spiral arms. The galaxy appears relatively isolated, with no obvious signs of major gravitational interaction or merging activity. Subtle disturbances may be present.
