The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There are no readily apparent spiral arms or distinct features such as dust lanes or star-forming regions visible. The light profile shows a gradual decline in intensity from the center outwards. The color appears relatively uniform, with a yellowish hue, suggesting a population of older stars. The overall shape is somewhat elongated, falling somewhere between round and cigar-shaped. There is no visible evidence of ongoing mergers or major tidal disturbances affecting the structure of the galaxy.
