The galaxy exhibits a generally diffuse morphology. The central region is brighter and more condensed, suggestive of a galactic nucleus. The overall color is bluish, potentially indicating active star formation within the galaxy. The galaxy appears somewhat asymmetrical and potentially irregular. There seems to be evidence of possible tidal distortions or interactions. The galaxy's shape departs noticeably from a simple elliptical or spiral form. There are no clearly defined spiral arms or a prominent disk structure visible in this observation.
