The galaxy presents as a moderately bright, unresolved object. It has a nearly circular morphology, though with some irregular edges. The color distribution suggests a dominant central region with a bright, blue-white core, indicating a population of young, hot stars. Fainter, more diffuse material surrounds the core. There may be some evidence of faint spiral structure or disk features, though this is difficult to ascertain. A slight asymmetry in the outer regions is visible and may suggest the presence of a minor disturbance, possibly a gravitational interaction or ongoing merger event. Overall, the galaxy appears to be relatively compact. 
