This galaxy exhibits a generally rounded morphology, with a somewhat smooth appearance overall. The central region presents a bright, concentrated core that diffuses outward. There is an indication of possible tidal disturbances or asymmetries in its outer structure, with subtle extensions emanating from its core region. The color gradients suggest a distribution of stellar populations, with bluer hues on one side of the galaxy possibly indicating areas of more recent star formation, and a redder concentration present on the other side. The red could also be indicating increased dust concentration in that area. Some subtle distortions appear to be present, warranting further investigation to determine if the galaxy is undergoing a minor merger event. 
