The galaxy presents as a moderately bright, centrally concentrated object. The primary color appears to be a warm yellow-orange, suggestive of an older stellar population. The light profile indicates a smooth morphology, with a high degree of radial symmetry. There is a hint of elongation, but the isophotes are predominantly elliptical, tending towards circular. There is no obvious spiral arm structure or dust lane visible within the resolution limits of the image. Subtle irregularities in the outer regions of the galaxy may indicate minor tidal disturbances or past interactions.
