The galaxy presents a flattened, disc-like morphology with a prominent central bulge. The core region exhibits a bright, relatively smooth appearance, possibly indicating an older stellar population. Surrounding the core, there is evidence of a fainter, more diffuse disc structure. The colour gradients suggest a radial variation in stellar populations or dust content, with a bluer outer edge of the disc. There are indications of faint, disturbed features, suggesting a possible interaction or past merger event. These disturbances do not appear to be strongly disruptive, but instead appear to be mild irregularities. There is no defined spiral structure that is obvious, but this is not to say it is completely absent.
