The galaxy presents a largely smooth visual appearance, with a high probability of being classified as smooth. The overall shape is generally described as intermediate in roundness, neither perfectly circular nor highly elongated. There is a low probability of a cigar-like shape. A small fraction of light is disk-like. While the galaxy primarily exhibits a non-disturbed morphology, there is evidence to suggest that it may be undergoing or have undergone minor disturbances, with a small chance of it being a major merging event or merger remnant. The galaxy exhibits a color gradient, with bluer hues on the outer edges and a redder core. Overall, the galaxy presents a moderate level of star formation.
