The galaxy presents with a moderate degree of internal structure. The overall form is not entirely smooth; there is evidence of features within the galactic disk. There appear to be some disturbances, possibly indicative of a minor merger event. The light distribution suggests a spiral structure, though it is not well-defined, with hints of arms. There are areas of active star formation, noted by regions with a slightly bluer hue, and more extended regions with older stars. The galaxy is not perfectly circular; there are some irregularities in its overall shape, adding to the suspicion of some interactions. The galaxy appears to be of average size and luminosity.
