The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of central concentration. There is a slight elongation, though it is predominantly round. The light profile appears relatively uniform across the galaxy's surface, suggesting a lack of prominent spiral arms or distinct substructures. There is a hint of a tidal disturbance or possible merger, though it is not immediately clear. The galaxy appears to be generally red in color, which indicates that the galaxy is mostly composed of older stars. Given this information, the galaxy has low star formation rate.
