The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-white, suggesting a population of older stars. The galaxy appears elongated and slightly cigar-shaped, with a diffuse halo extending beyond the central region. There is no visible evidence of spiral arm structure or significant dust lanes. Faint, subtle irregularities in the outer regions may hint at minor gravitational interactions or disturbances, but no major merger event is apparent. The overall color suggests a relatively low rate of ongoing star formation within the galaxy.
