The galaxy presents as a centrally concentrated object, exhibiting a smooth, relatively featureless morphology. The central region displays a high degree of luminosity, suggesting a dense stellar population or possible active galactic nucleus. The light from the galactic center fades gradually outward. The galaxy appears largely elliptical or lenticular in shape with only a suggestion of a disk. There is no strong evidence of ongoing major mergers or tidal disturbances, although a slight asymmetry may suggest a minor interaction in its past. The galaxy exhibits a warm color, consistent with an older stellar population and suppressed star formation. 
