This galaxy presents an irregular morphology. A prominent, bright, centrally located region exhibits a blue-green hue, potentially indicating a high concentration of hot, young stars or significant ionized gas activity. A less luminous, extended structure curves away from this central region, showing a gradient of color from bluish-white to a faint redder tint along its path. The extended structure appears somewhat clumpy, suggesting possible star-forming regions or dust lane concentrations. In addition, a separate yellow region is present underneath the central bright blue region, and may be a source of older redder stars. The overall structure suggests the possibility of a galaxy undergoing tidal disruption or an interaction with another galaxy, though the immediate presence of a clear merging partner is not obvious in this image. The galaxy's morphology does not fit neatly into typical elliptical or spiral classifications.
