The galaxy presents as a luminous, centrally concentrated object with a generally smooth appearance. Its overall morphology appears to be elliptical, with a round shape. The central region exhibits a yellowish-white hue, suggesting an older stellar population. Fainter, diffuse blue light is visible in the outer regions, indicative of some younger, hotter stars, though this is minimal. There is a faint hint of a disk structure. No major tidal features or signs of ongoing mergers are readily apparent, however there is some minor disturbance. 
