The galaxy presents as a centrally concentrated object. The light profile appears smooth with a round morphology. There is a slight elongation, but the overall shape is close to circular. The color index suggests a redder stellar population, potentially indicating an older system with a relatively low rate of on-going star formation. The galaxy shows no obvious signs of tidal disturbances or interactions with neighboring galaxies. There is evidence of faint extensions, but these could be due to noise.
