The galaxy presents as a somewhat irregular object, elongated in shape, with a brighter, concentrated central region that may suggest a nucleus or bulge. There is a hint of a spiral arm-like structure emanating from the central region, but the arms appear diffuse and indistinct, possibly indicating a disrupted morphology. The overall color of the galaxy is bluish-white, suggesting a population of relatively young, hot stars. There are also some redder regions that may indicate the presence of dust or older stellar populations. No obvious signs of a major ongoing merger are immediately apparent, but some minor disturbances or tidal features might be present, warranting further investigation. The galaxy exhibits a moderate surface brightness, indicating it is neither exceptionally bright nor faint for a galaxy at its estimated distance.
