The galaxy appears to be a disk galaxy, viewed at a moderately inclined angle. It exhibits a central bulge region that is brighter and more concentrated than the outer disk. The overall color is bluish, suggesting ongoing star formation. While the disk structure is apparent, it appears somewhat disturbed or irregular, hinting at possible interactions or past mergers. There are subtle features within the disk, possibly indicating spiral arm segments. There are signs of slight tidal disturbances on one side of the galaxy. The galaxy appears relatively compact.
