The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of concentration, appearing as a bright, nearly uniform core. Progressing outwards from the core, the intensity of light gradually decreases, forming a diffuse halo. There's no clear indication of spiral arms or significant dust lanes. The overall color appears to be somewhat redder, possibly indicating an older stellar population with suppressed star formation, compared to typical spiral galaxies. The galaxy has an elongated shape.
