The galaxy appears to be a spiral galaxy, observed at a relatively low inclination angle. There is a distinct central bulge, with the majority of the light concentrated in a somewhat elongated spheroidal region. While the image resolution is limited, faint spiral arm structures are suspected. These arms seem loosely wound, with a prominent two-arm spiral structure. The galaxy exhibits disk features, with a clear distinction in color between the inner bulge and the outer disk, which appears bluer than the bulge. No signs of a significant merger event are immediately visible, suggesting that if there are minor interactions these are in early stages. A bar is present across the galaxy with a moderate strength.