The galaxy presents as a relatively smooth, elliptical structure. There is a clear central bulge, slightly elongated, with a somewhat diffuse outer halo. The color profile indicates a redder core, suggesting an older stellar population, surrounded by a halo that appears to be relatively bluer. The galaxy exhibits an intermediate roundness, leaning towards being in-between round and cigar-shaped. No significant signs of spiral arms, dust lanes, or major disturbances are apparent in this observation, but there may be some minor perturbations.
