The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. It exhibits a relatively high degree of symmetry, although there is a slight elongation visible along what appears to be its major axis. The light distribution is centrally concentrated, with a gradual falloff in intensity towards the outer edges. Color gradients suggest a possible redder population of stars concentrated towards the core, with bluer light extending further into the galaxy's halo. There is little to no evidence of spiral arms, distinct dust lanes, or significant star-forming regions within the visible portion of the galaxy. Overall, the galaxy appears to be relatively undisturbed.
