The galaxy presents as a relatively smooth, elliptical morphology with a centrally concentrated bulge. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. The light appears to gradually diminish in intensity as one moves outward from the center towards the galaxy's edge. The color shifts subtly toward a greenish-blue tint within the outer regions, possibly indicating a slight presence of younger stars or ionized gas, however, star formation is likely low. No distinct spiral arms or bar features are discernible within the resolution limits of this image. There are no indications of any major mergers or tidal disturbances affecting the galaxy's structure, though minor disturbances cannot be ruled out. The galaxy appears largely undisturbed and generally round in shape, with a slight ellipticity. The estimated size suggests a substantial but not extreme galactic dimension.
