The galaxy presents an apparently disturbed morphology. It is somewhat diffuse with an asymmetric distribution of light. There is a slightly brighter, more compact central region. The overall color appears reddish, indicating a possible population of older stars, particularly when considering the relatively low blue light. There is a slight indication of some disruption possibly due to a merger, with a slight asymmetry noted. The shape is irregular, not a well defined spiral or elliptical.
