This galaxy presents as a relatively compact object. There is a bright, centrally concentrated region, likely representing the galactic nucleus. The galaxy appears to have a disk-like structure extending outwards from the central region, but is poorly defined. There is some evidence of minor disturbances or irregularities in the outer regions of the disk. Overall, the galaxy exhibits a mostly smooth appearance, but not entirely featureless. Some faint traces of what appear to be spiral arm segments can be discerned within the disk, although they are not clearly defined or prominent. Colors range from a bright central white to a slightly blueish tint in the outer regions of the disk. Indications of a possible merger event are present, and its overall structure is not regular, implying ongoing gravitational interactions.
