The galaxy presents as a roughly elliptical, centrally concentrated object. Its core region exhibits a higher surface brightness, appearing almost unresolved. There is a moderate colour gradient observed, with the core showing a tendency towards redder hues.

Surrounding the core, the outer regions exhibit a bluer hue. Some faint patches, suggestive of stellar populations or nebulae, are present but indistinct. The galaxy's outer boundaries lack sharp definition, fading gradually into the background. No prominent spiral arms or bar structures are readily visible. There appears to be no signs of strong interactions or recent major mergers. The galaxy appears to be relatively compact in size.
