The galaxy presents an overall ellipsoidal morphology, appearing largely smooth and relatively compact. A bright, centrally concentrated region exhibits a bluish-white hue, possibly indicating the presence of a population of young, hot stars and ongoing star formation. Surrounding this core, a more diffuse, yellowish halo is visible. This halo might represent an older stellar population. A ring-like structure, more prominently blue and bordering on violet in color, encircles the central core. This could be an area of intense star formation. There is a hint of a more extended, faint outer region that could denote a larger galactic structure, although this is difficult to discern clearly from the image. The galaxy does not appear to be undergoing a major merger, but subtle disturbances or minor irregularities in the overall structure cannot be ruled out. The smoothness and color distribution suggests that the galaxy may be a lenticular or early-type spiral galaxy, though lacking definitive spiral arm features.
