The galaxy presents a roughly elliptical morphology with a disk-like component. A slight yellow hue concentrates toward the center of the galaxy, likely indicating an older stellar population and dust concentration within the central region. The outer regions display a bluer color profile suggesting areas of active star formation within its spiral arms. The galaxy exhibits signs of disturbance, potentially due to a past or ongoing minor merger event. Overall, the galaxy appears as a luminous system with a considerable stellar mass.