The galaxy appears as a moderately luminous object with a roughly elliptical morphology. The light distribution is centrally concentrated, with a smooth, diffuse appearance. There is a subtle color gradient, transitioning from a bluer hue in the outer regions to a redder hue toward the central bulge. There are hints of a faint, extended disk, although it is not sharply defined. No distinct spiral arm structure is readily apparent, suggesting a relatively quiescent galaxy. Subtle disturbances or asymmetries may be present, indicating a possible interaction or merger event in the galaxy's past or ongoing.
