The galaxy presents as an elliptical structure with a smooth, diffuse light distribution. It displays a pronounced central bulge that is elongated in shape, appearing somewhat cigar-like. The core exhibits a yellowish-white hue, suggesting a population of older stars. There is little to no evidence of spiral arm structure or dust lanes. The galaxy appears relatively isolated, with a faint companion object visible nearby on the right side of the galaxy. There does not appear to be any major merging activity affecting its structure. The overall color indices suggest a higher concentration of stellar mass with relatively low ongoing star formation.