The galaxy presents as a slightly elliptical, yellowish core region. There are hints of spiral arm structures, though they appear faint and somewhat disrupted. Several distinct, brighter knots of redder light are visible within the disk, possibly indicating regions of active star formation or dust concentrations. Overall, the galaxy's morphology suggests a mature system, potentially undergoing some form of interaction or disturbance. The light profile seems relatively smooth in the central region, with the apparent disturbances concentrated within the outer disk.
