The galaxy presents as a generally elliptical structure with a smooth, diffuse morphology. The central region exhibits a high concentration of light, indicative of a significant stellar population and potentially a supermassive black hole at the core. There is no apparent bulge or spiral arm structure discernible in the image. The overall color profile suggests a population of older stars, with a yellowish-red hue dominating. There is no dust lane visible or indication of significant recent star formation. The object appears isolated, with no clear evidence of tidal interactions or ongoing mergers with other galaxies. The general shape appears to be slightly more round than elongated. Any disturbances are minor, and the disk fraction is low. 
