The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. It appears to be largely featureless, lacking prominent spiral arms or distinct substructures. The light distribution suggests a high degree of rotational symmetry.

The color gradient indicates a redder core, transitioning to slightly bluer hues in the outer regions. This might reflect an older stellar population concentrated towards the center, with younger, bluer stars more prevalent in the galaxy's periphery. The overall reddish color indicates a low rate of on-going star formation. There are no obvious signs of an active galactic nucleus or intense starburst activity based on the broad color information. The shape shows no indication of a major merger event, but there is the possibility of a minor disturbance in the even distribution of the galaxy.
