The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse appearance. The color profile suggests a bulge that transitions from a redder core to a slightly bluer halo. There is no apparent spiral arm structure or distinct disk component. The object exhibits a somewhat elliptical shape. There is a minor disturbance visible, but the galaxy is not undergoing a major merger. The estimated size of the object suggests that the light emanates from a galaxy of considerable diameter. The star formation rate appears to be relatively low.
