The galaxy presents a generally smooth and elliptical morphology. The light is centrally concentrated, exhibiting a bright, yellowish core that fades into a less luminous halo. There is no obvious spiral structure or prominent dust lane visible within the galaxy. The shape tends toward being in between round and elliptical, lacking a highly elongated or cigar-like appearance. There is no indication of ongoing major merger events. Subtle irregularities or minor disturbances may be present, but are not pronounced, and the system is generally undisturbed. The overall color suggests an older stellar population.