The galaxy appears to be a spiral galaxy, though the classification is somewhat uncertain. It exhibits a moderate degree of central concentration, with a bright, well-defined nucleus. The spiral arms are not sharply defined; instead, they appear somewhat flocculent and patchy, suggesting ongoing or recent star formation. The galaxy is likely viewed close to face-on. There is some irregularity or distortion visible in its outer regions that could be the result of a minor interaction with another galaxy. The morphology is somewhat smooth, so there is not a strong central bulge like a typical spiral galaxy. The disk, however, appears more prominent than the bulge. There might be minor disturbances visible in the galaxy.
