The galaxy appears as a concentrated, elliptical-like structure. It exhibits a smooth, relatively featureless morphology, lacking prominent spiral arms or significant dust lanes. The central region is a bright yellow, indicating a high concentration of older stars. The outer regions show a transition to slightly bluer hues, suggestive of a younger stellar population. Overall the galaxy is of average size and mass and shows no evidence of a major merger or tidal disturbance. 
