The galaxy presents a generally smooth, elliptical morphology. Its core appears bright and concentrated, displaying a yellowish hue suggestive of an older stellar population. The isophotes are relatively regular, hinting at a relaxed dynamical state. There is a subtle color gradient from the core to the outer regions, with the outer halo appearing slightly bluer. This might indicate a small amount of ongoing star formation or the presence of younger stars in the outskirts. No strong tidal features or evidence of recent mergers are readily apparent in the immediate vicinity, although there may be a small disturbance on one side of the galaxy. The overall appearance is consistent with a massive galaxy that has largely ceased active star formation.
