The galaxy presents as a flattened elliptical shape, with an apparent major axis orientation approximately northeast to southwest. There is a bright, concentrated central bulge that dominates the overall luminosity profile. The galaxy exhibits a smooth, diffuse halo that gradually fades into the background sky. The color appears generally redder, suggesting a population of older stars with less ongoing star formation. There may be a slight warp or asymmetry in the outer disk, although this could be due to image artifacts. There's no strong evidence of prominent spiral arms or dust lanes within the galaxy.
