The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge, indicative of a significant stellar population within the core. The overall color appears yellowish-white, suggesting a dominant population of older stars. There is a subtle elongation to the galaxy's shape, appearing slightly cigar-shaped. No distinct spiral arms or obvious dust lanes are visible. Faint hints of possible minor disturbances are present within the extended halo, but these are not pronounced. The light profile appears centrally concentrated, with brightness decreasing steadily outwards from the core.
