The galaxy presents as a disturbed system, potentially undergoing a merger. The morphology is complex, showing characteristics of both smooth and disk-like structures. A significant portion of the galaxy appears smooth with the remainder having features of a disk. There is a bright, yellowish central region, possibly indicating an older stellar population or an active galactic nucleus. A blue-ish region is visible, suggesting areas of more recent star formation. The overall shape is somewhat elliptical but distorted, with asymmetries in the distribution of light. The galaxy may be undergoing a major merger, with signs of tidal features.