The galaxy presents as a largely featureless, smooth object. It appears elliptical in shape, with a high degree of roundness. The core region exhibits a strong concentration of light, suggestive of a relatively old stellar population. The color profile indicates a concentration of older, redder stars, with a subtle gradient towards bluer hues in the outer regions. There are no apparent spiral arms, bars, or other significant morphological disturbances. No major merging signatures are evident.
