The galaxy appears as a relatively compact, elliptical-like object with a smooth, centrally concentrated light profile. It exhibits a yellowish-white hue, suggesting an older stellar population with relatively low ongoing star formation. There is a slight color gradient, with the central region appearing more yellow than the outer regions, possibly indicating a higher concentration of older stars in the core. There are no distinct spiral arms or prominent dust lanes visible. Overall, the galaxy’s morphology suggests it is a relatively massive, early-type galaxy. There is an apparent absence of any significant tidal features or signs of recent major mergers, suggesting it is a relatively undisturbed system.
