The galaxy presents an elliptical morphology, appearing somewhat elongated but generally smooth in structure. There is a noticeable central bulge that appears to be composed of older stellar populations, indicated by its yellowish-orange hue. The disk component, though present, lacks prominent spiral arms, suggesting it is relatively featureless or that the galaxy is transitioning from a spiral to an elliptical form. Some subtle disturbances can be observed, suggesting potential tidal interactions or past merger events, though no distinct tidal tails are readily apparent. There is some evidence of active star formation taking place, this is subtle but can be inferred from the blue tinged color and the disturbances in the galaxy. Overall, the galaxy appears to be intermediate in type, possibly an early-type spiral or a late-type elliptical.
