The galaxy presents as a relatively smooth, centrally concentrated object. Its shape appears to be roughly elliptical, deviating slightly from a perfectly circular morphology. A slight elongation is observed. The core region exhibits a yellowish hue, suggesting a population of older stars. The outer regions of the galaxy are fainter with a hint of blue, potentially indicating the presence of a younger stellar population, but this is not definitive. No prominent spiral arms or distinct features are apparent. Faint distortions seem to be present, suggestive of minor disturbances, potentially indicative of interactions or mergers in the galaxy's past. No definitive signs of ongoing major merger events are present.
