The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outwards, transitioning into a fainter halo. The overall color appears yellowish-orange, suggesting a population of older stars with minimal ongoing star formation. There is a slight deviation from perfect circularity, with a hint of a cigar-shaped structure and a mild disruption. No prominent spiral arms or significant dust lanes are discernible. The lack of blue color indicates it is relatively inactive, with a low specific star formation rate.