The galaxy appears as a single, relatively smooth, concentrated object. The light is centrally concentrated and the overall morphology exhibits a generally elliptical shape. The galaxy shows a gradual decrease in brightness from the core to the outer regions, lacking any distinct spiral arm structures or prominent features typically associated with disk galaxies. There are no signs of a strong tidal disturbance, close companions, or significant ongoing merger activity. The color of the galaxy appears somewhat red, indicative of an older stellar population with limited ongoing star formation, though there is a slight amount of bluer light emanating from the center of the galaxy.
