The galaxy appears as a relatively smooth, somewhat elliptical structure. Its light is centrally concentrated, suggesting an older stellar population in the core. Fainter, diffuse light extends outward from the central region, hinting at a possible disk or envelope. There is a slight asymmetry in the outer isophotes, possibly indicating a minor gravitational interaction or past merger event. The overall color appears to be relatively uniform, with a subtle redder hue compared to bluer spiral galaxies.
