The galaxy appears to be a spiral galaxy, viewed at an oblique angle. The central bulge is somewhat bright and moderately sized, with a slightly elongated morphology, suggesting the possible presence of a weak bar structure bisecting the core. Spiral arms are visible, extending from the central region, and are not tightly wound, displaying a somewhat flocculent structure with regions of active star formation visible as bluer knots along the arms. There is some indication of dust lanes visible in the arms. The overall color suggests a mixed stellar population, with both older, redder stars and younger, bluer stars. The outer regions of the disk fade into the background, and the galaxy does not show any obvious signs of a major merger.
