The galaxy presents as a moderately bright, centrally concentrated object with an elliptical morphology. Its light profile appears relatively smooth, lacking obvious spiral arms or distinct features suggestive of active star formation. The color gradient transitions from a bluer hue at the core to redder shades towards its outer regions. The core exhibits a fairly uniform intensity distribution, while the outskirts gradually fade into the background. No evidence of tidal streams or other indicators of recent major mergers are visually discernible. The overall appearance suggests a well-evolved system, possibly an elliptical galaxy dominated by an older stellar population. Minor asymmetries are subtle.
