This galaxy exhibits a clear spiral structure, with two prominent arms emanating from a central bulge. The spiral arms are relatively well-defined and appear to be moderately wound. The arms display a clumpy morphology, suggesting active star formation regions. The galaxy has a flattened disk and the bulge appears to be small relative to the overall disk size. There is no obvious bar structure visible. The overall color is somewhat blue, indicative of a stellar population with a significant fraction of young, hot stars. There are minor disturbances or irregularities present in the disk, which could be a result of a recent or ongoing minor merger event.
