This galaxy presents as a single, extended object with a somewhat irregular morphology. A dominant, bright core region is visible, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. This core appears slightly offset from the apparent center of the overall galactic structure.

Surrounding the core, a fainter, diffuse halo extends outward, displaying a bluer coloration. This suggests the presence of a younger stellar population or ongoing star formation within the outer regions. There appears to be a significant level of disturbance on the left side of the galaxy. Possibly the beginning of a tidal tail extending from the core.

Overall, the galaxy shows clear asymmetry and signs of interaction or internal processes that are disrupting its structure. The morphology suggests a possible ongoing merger event or the aftermath of a previous interaction.
