The galaxy presents an elliptical morphology, with a centrally concentrated, smooth light distribution. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the light intensity gradually decreases, and the color shifts subtly toward a reddish tone, potentially indicating the presence of evolved stars and dust. The galaxy's overall shape is slightly elongated. No distinct spiral arms or bar structures are visible. A minor asymmetry may be present in the outer regions, but the primary structure appears largely undisturbed.
