The galaxy presents as a relatively compact object, exhibiting a morphology that appears largely smooth. There is a slight deviation from perfect circularity, leaning towards an elliptical shape, although it is not highly elongated. The light is concentrated towards the center, suggesting a prominent central bulge. There may be some slight disturbances visible in the galaxy's structure, potentially indicative of minor gravitational interactions or past merger events. There does not seem to be much star formation occurring within the galaxy.
