The galaxy appears as a relatively smooth, somewhat rounded object. It exhibits a concentrated central region, with an extended halo of diffuse light surrounding it. There is evidence of a slightly disturbed morphology, potentially indicating an ongoing or past merger event. Within the galaxy's structure, we observe a mix of stellar populations, evident from the color variations. Yellowish hues dominate, suggestive of older stellar populations, while subtle reddish components hint at regions of active star formation or dust obscuration.
