The galaxy presents as a relatively small, moderately bright object with a flattened, elongated shape. A bulge region is discernible in the center, appearing more concentrated and brighter than the surrounding disk. The disk structure is somewhat ill-defined and shows a clumpy texture, potentially indicative of regions of active star formation. The color is generally bluish, suggesting the presence of a young stellar population, but the bulge appears slightly yellower, which could be due to an older stellar population. Overall, the galaxy appears to be a late-type spiral or possibly an irregular galaxy with a notable central bulge.
