The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests a population of older stars, concentrated toward the center and producing a yellowish hue. A faint, diffuse bluish halo surrounds the central region, potentially indicating a small amount of ongoing star formation or a population of younger stars that are more dispersed. The galaxy appears relatively undisturbed, exhibiting no obvious signs of tidal interactions or major mergers. Its overall shape is more disc-like than cigar shaped. The galaxy appears to have a low to intermediate rate of star formation.
