The galaxy appears as a somewhat rounded, centrally concentrated object with a diffuse halo. The primary color is a pale blue, suggesting the presence of a population of young, hot stars and ongoing star formation. However, the overall light distribution seems relatively smooth, lacking the distinct spiral arm structures typically associated with actively star-forming galaxies. There are hints of disturbances, but the galaxy has not fully merged with another. The morphological characteristics suggest this galaxy is somewhere between an elliptical and spiral galaxy in terms of its structure and likely its evolutionary state.
