This galaxy exhibits a morphology that is neither purely elliptical nor a well-defined spiral. A central bulge is visible, though it appears relatively indistinct. The galaxy appears somewhat elongated. Blue-ish regions are visible, possibly indicating areas of active star formation, although the overall structure is not clearly defined as a spiral disk. There is evidence of possible disturbances in the galaxy's structure, hinting at a possible interaction or merger event. The appearance suggests a galaxy that may be in the process of merging with another, or recently underwent a merger.
