The galaxy presents as a centrally concentrated object with a smooth morphology. It exhibits a relatively round shape, with minimal deviation towards an elongated form. There is a slight indication of a disk-like structure. No major disturbances or mergers are immediately apparent, although subtle asymmetry is present within the galaxy's outer regions. The central region appears predominantly yellow, suggesting an older stellar population, while the outer parts show a slight bluer tint, hinting at younger stars.