The galaxy presents as a relatively smooth, centrally concentrated object. There is some indication of a disk structure, but no clear spiral arms or bar are visible. The morphology appears somewhat rounded, though it is not perfectly spherical. There may be ongoing or recent merger activity. There appears to be higher levels of star formation indicated by the more blue color to the top-left of the galaxy, which could be due to tidal interactions and recent gas compression causing star formation. The mass of the galaxy appears to be moderate.
