The galaxy presents a flattened, elliptical morphology. It exhibits a diffuse, relatively smooth luminosity profile, suggesting a lack of prominent spiral arm structure. The color appears primarily bluish-white, indicative of a stellar population with a significant fraction of young, hot stars, and the galaxy may exhibit ongoing star formation, concentrated towards the center of the galaxy. There is also a component of more yellow light towards the center of the galaxy, which could indicate an older population of stars. There is no clear evidence of a recent major merger, though some subtle disturbance in the outer regions may suggest a past interaction or minor merger event.
