The galaxy appears to be a spiral galaxy, presented at an oblique angle relative to our line of sight. There is evidence of spiral arm structure, although not sharply defined. One arm appears prominent, beginning to the left of the central bulge and extending upwards, with a slightly mottled and fragmented morphology. There appears to be an arm located on the right-hand side of the galaxy, as well.

The central bulge appears moderate in size, with a concentrated central intensity that decreases gradually towards the outer regions of the galaxy. The disk surrounding the bulge is visible, with a flattened structure that exhibits some irregularities. There are some noticeable light variations and color changes in this disk.

There appears to be a tidal tail or stream extending from the galaxy, which could imply a gravitational interaction with another galaxy. Overall, the galaxy shows a mix of smooth, bulge-dominated regions and more irregular, star-forming disk components.
