The galaxy presents as a somewhat elliptical, moderately concentrated light source. A brighter central region is apparent, possibly indicating a galactic nucleus. Diffuse light extends from the central region, with a possible tail like structure stemming off the bottom. The light is noticeably blue, suggesting the presence of hot, young stars and active star formation. There appears to be some disruption of the overall structure, possibly hinting at a past or ongoing interaction with another galaxy.
