The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The light profile appears to lack distinct features such as spiral arms or a prominent bar. The core exhibits a bright, yellowish hue that gradually fades into a fainter, reddish outer region. There is a slight ellipticity to the overall shape, but it is mostly round. No obvious signs of tidal disturbances or ongoing mergers are visible, although subtle irregularities in the outer envelope cannot be entirely ruled out. Given the apparent color and lack of prominent star-forming regions, it is likely composed predominantly of older stellar populations.
