The galaxy exhibits a disturbed morphology, possibly indicative of an ongoing or recent interaction. A central, somewhat elongated, concentration of older stars is present, appearing yellowish-orange in color. This suggests a substantial population of evolved stars within the galactic bulge. Surrounding this central region, there are hints of blue patches, which could be regions of ongoing star formation. The overall structure appears irregular, with no well-defined spiral arms or elliptical shape. There may be some tidal features or faint extensions, particularly to the upper left, that contribute to the galaxy's irregular shape, further supporting the hypothesis of a merger event. Based on its color, this galaxy may be in a transitional state between a spiral and elliptical galaxy, although the exact nature of the morphological transformation is unclear from this image alone.
