The galaxy presents a largely featureless morphology, appearing as a single, smooth concentration of light. It is roughly elliptical in shape, though nearly circular. The central region exhibits a higher surface brightness, with the intensity gradually decreasing towards the outer edges. The color profile suggests a population of older stars, as indicated by the yellow-red hue. There is no readily apparent spiral structure, nor any obvious signs of ongoing mergers or tidal disturbances. The overall appearance is consistent with a relatively evolved system. 
