This galaxy presents a roughly elliptical morphology. The core region is a bright, condensed structure, exhibiting a pale blue hue suggestive of elevated rates of star formation or a population of hot, young stars. Surrounding this core, the galaxy displays a fainter, more diffuse halo, which appears marginally extended. There may be some evidence of minor distortions or irregularities in the outer regions of the disk, but the galaxy appears largely undisturbed. The color gradient transitions from a blue-dominant central region toward more greenish and reddish tones in the outer disk, which may indicate an older stellar population at larger radii or dust obscuration. 
