The galaxy presents a morphology that suggests it is likely a spiral galaxy, exhibiting a prominent disk-like structure. This disk shows evidence of internal structure, indicating the presence of spiral arms. The arms are somewhat disorganized, and there may be tidal disturbances, perhaps hinting at a past interaction or merger event. The central bulge is quite pronounced and relatively bright, potentially indicating an older stellar population. The color distribution within the galaxy suggests a variation in stellar populations and star formation activity, with bluer regions likely representing areas of active star formation and redder regions indicating older stellar populations. The overall color of the galaxy appears yellowish-white suggesting a mix of stellar populations. There appears to be another object in the vicinity which could be related or could be a foreground object. The galaxy appears to be relatively massive and is undergoing low levels of star formation.
