The galaxy presents a complex, irregular morphology, possibly indicative of an ongoing or recent interaction. A dominant, concentrated central bulge exhibits a yellowish-orange hue, suggesting an older stellar population and reduced recent star formation. The bulge is surrounded by a fainter, bluer disk component with hints of spiral structure. The disk is not sharply defined, displaying a more diffuse appearance. There are distinct areas of blue-shifted color, possibly representing increased star forming regions within the disk. The overall light profile shows a centrally concentrated source with a diffuse and asymmetric outer region.
