The galaxy appears to be an irregular-shaped system, displaying both smooth and clumpy features. A brighter, more diffuse region resides at the top, possibly indicating a galactic nucleus or a dense concentration of stars. A dust lane is not visible, but there are some more opaque regions.

The bulk of the galaxy is more diffuse, with a notable presence of blue regions suggestive of ongoing star formation within its body. These pockets of star formation are irregularly distributed, lending to the overall amorphous morphology. There are some indications of disturbances, such as faint tidal tails or asymmetrical structures within the system. These features suggest past or ongoing interactions with another galaxy, potentially a minor merger event contributing to its irregular structure.
