The galaxy presents as a somewhat diffuse, centrally concentrated object. It appears largely featureless, lacking prominent spiral arms or distinct morphological substructures. The color profile suggests a generally older stellar population with a dominance of redder wavelengths, although some bluer emission is present, indicating the possibility of ongoing, albeit subdued, star formation. The overall shape is roughly elliptical. There is no obvious sign of major mergers or tidal disturbances in its immediate vicinity, although there appears to be a slight asymmetry, possibly indicating a minor interaction in its past. 
