This galaxy appears to be in the process of merging. The primary body exhibits a smooth morphology and is slightly elongated. A smaller, bluish component is visible to the west, suggesting active star formation. To the east is a fainter, redder component which could be a tidal tail or another galaxy interacting with the main body. There is also a hint of disruption or asymmetry in the overall structure. The color index suggests a substantial population of older stars, but also ongoing star formation activity.
