The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears approximately circular, with a smooth transition in luminosity outward. The color gradient suggests a population of primarily older stars, with a yellowish-red hue dominating the visual spectrum. There is no discernable spiral arm structure or significant dust lane obscuration. Faint extensions of light are present, but they are subtle and do not represent a disturbed or actively merging system. The overall impression is that of a relatively quiescent, evolved galaxy.
