This galaxy exhibits a morphology that appears to be in transition. A central bright, compact, and relatively smooth component dominates the image. Surrounding this central region is a fainter, slightly irregular ring-like structure displaying a bluer hue. To one side of the central bright region is a more diffuse, elongated feature with a yellower color, which could be indicative of a disrupted spiral arm or tidal tail. The overall appearance suggests a possible interaction or merger event, evidenced by the distorted morphology and the presence of both a smooth central component and a disrupted disk-like feature. Star formation appears to be ongoing within the blue ring, while the yellower region may be older stellar populations. The galaxy has a substantial mass.
