The galaxy appears as a centrally concentrated object, likely an elliptical or lenticular type based on its smooth, featureless morphology. There's a distinct color gradient, shifting from a brighter, yellowish-white core to a bluer, fainter outer halo. The galaxy has a generally round appearance, with a slight elongation. No distinct spiral arms or dust lanes are discernible. There appears to be little to no evidence of tidal disturbances or recent major mergers, though some minor asymmetries in the outer regions might suggest minor interactions. The overall color profile suggests a population dominated by older stars, particularly in the central region.
