The galaxy appears to be a spiral galaxy, viewed at a high inclination angle. The central bulge region appears bright and relatively smooth, with a slightly elongated shape. Fainter, diffuse light is visible extending outwards from the bulge, tracing a more elongated disk-like structure. A slight asymmetry can be noted in the outer regions, possibly indicating minor disturbances or interactions with other galaxies. The color distribution indicates varying stellar populations within the galaxy. The central region appears whiter, possibly indicating older stars, while the fainter outer regions appear more blueish-green, which could be due to younger, hotter stars.
