The galaxy appears to be a relatively smooth, centrally concentrated object. The morphology seems to be predominantly elliptical with little to no discernible spiral structure. The galaxy exhibits a color gradient, with a more yellowish-red hue in the central region, potentially indicating an older stellar population. The outer regions fade into a more blueish hue suggesting some low level star formation may be ongoing. There is no evidence of major disturbances or ongoing mergers; the galaxy appears relatively undisturbed. The galaxy's shape is predominantly round and fairly compact.
