The galaxy presents as a slightly elongated, lenticular structure. It has a bright central bulge that gradually fades outward into a diffuse disk. The light from the galaxy appears relatively smooth, showing a subtle gradient from yellow-white to light blue hues. The central region has a warm yellowish colour, suggesting an older stellar population, while the edges have hints of cooler blue, which suggest ongoing but minimal star formation. There is no evidence of spiral arms or active galactic nuclei. No signs of a significant ongoing merger activity are observed, though possible disturbances cannot be entirely ruled out. Overall, the galaxy appears to be a fairly evolved system.
