The galaxy presents as a somewhat elongated, elliptical structure with a bright, concentrated central bulge. There is a smooth appearance to the galaxy's light distribution, suggesting a relatively old stellar population dominating the luminosity. A faint, diffuse halo surrounds the central region, extending further along the major axis. There is no strong evidence of spiral arms or prominent dust lanes. Subtle color variations can be discerned, with a slightly bluer tint toward the outer regions of the halo, suggesting some ongoing star formation. The overall color is consistent with an intermediate to redder stellar population, typical of early-type galaxies at moderate redshifts. A potential tidal feature can be observed at the right side of the galaxy, which could indicate a past merger event.