The galaxy appears as a centrally concentrated object, with a relatively smooth, amorphous morphology. There is a slight elongation to its shape, presenting as somewhat elliptical. The light distribution suggests a lack of significant spiral arm structure or strong tidal features. The galaxy exhibits a color gradient, appearing more blue towards its core region and more red in the outer regions. Based on the redder color in the outer portions, it is suspected to be an older stellar population, while the core likely includes a younger stellar population. There are no immediately apparent signs of significant ongoing mergers or major disturbances to its structure, and a lack of strong dust lanes. The galaxy is a relatively compact object.
