The galaxy presents as a relatively compact, elliptical-like structure. The overall color appears to be a pale blue, suggesting the presence of a younger stellar population, but this is a very slight blue and could be contamination from the blue channel on the image. The light distribution is concentrated towards the center, exhibiting a smooth, centrally condensed morphology with a lack of distinct spiral arms or features. The galaxy has a fuzzy profile at the edges, which could be the result of a smooth decline in stellar density with increasing radius, or a result of the image processing. There is no evidence of ongoing major mergers or tidal disturbances, however there may be minor irregular features present. The axial ratio indicates it is not perfectly spherical, exhibiting a moderate flattening.
