The galaxy appears to be a spiral galaxy viewed at an oblique angle. The central bulge is prominent and appears yellowish, suggesting an older stellar population. The disk shows some evidence of spiral arm structure, though the resolution limits a clear view. The spiral arms appear somewhat patchy, with some bluer regions that could indicate areas of active star formation. The overall color suggests a mix of stellar populations, with an older, more evolved population dominating in the bulge and younger, hotter stars present in the spiral arms. The galaxy exhibits a somewhat elongated shape, and the presence of some diffuse light extending beyond the main body may suggest a halo of older stars or tidal debris from past interactions. There isn't much evidence for a current major merger, but some minor disturbances may be present.
