The galaxy presents as a disk-shaped system, viewed at an oblique angle to our line of sight. The central region appears to be dominated by an older stellar population, indicated by its yellowish-orange hue. Evident distortion suggests possible ongoing or recent merger activity. The overall structure appears disturbed, lacking the smooth, symmetrical morphology of a relaxed spiral or elliptical galaxy. Faint, elongated tidal features are visible extending from the main body, further suggesting gravitational interaction with another galaxy. There appears to be an object nearby which is a bright yellow blob, possibly the core of another galaxy that is in the process of merging. The disk also contains some bluer regions suggestive of star formation.
