The galaxy presents as a relatively compact object with a generally smooth appearance. A subtle disk-like structure is tentatively visible, presenting an elongated shape. There is evidence of an ongoing interaction or disturbance. There is an indication of possible tidal tails or faint plumes emanating from the galaxy's main body. The central region appears brighter and bluer, suggesting the presence of a population of younger, hotter stars. Overall, this galaxy appears to be in a state of transition, possibly due to internal processes or external influences.
