The galaxy exhibits a disturbed morphology, possibly indicative of an ongoing or recent interaction or merger event. A central, more luminous region shows a yellowish hue, suggesting an older stellar population. Extending from this central region are fainter features; it is difficult to discern distinct spiral arms, but some asymmetry is present. There appears to be a secondary concentration of light to the side of the central region, this could be another galaxy in the process of merging. The overall color gradients suggest a mixture of stellar populations, with some bluer regions that potentially indicate areas of active star formation, though these are not sharply defined. There is a slight reddening toward the center, possibly due to the accumulation of older stars or dust obscuration. The structure is not highly ordered, hinting at dynamical processes disrupting the galaxy's regular morphology.
