The galaxy presents a largely smooth, elliptical morphology, exhibiting a concentrated central bulge. Its overall color profile indicates an older stellar population, with a dominant yellowish-orange hue. There is faint light surrounding the central bulge, but there are no apparent spiral arm structures or significant dust lanes, suggesting a relative lack of ongoing star formation. The galaxy appears relatively isolated, with no obvious signs of a recent major merger. The slight asymmetry in its outer isophotes could indicate a minor interaction, but the predominant impression is one of an evolved, relatively quiescent system.