The galaxy presents a largely smooth, elliptical morphology. The light distribution is centrally concentrated with a gradual decrease in brightness towards the outer regions. There is a hint of a disk structure, though it is not sharply defined. The galaxy appears to be relatively isolated, showing no strong signs of interaction or major disturbances in its overall structure. The color is moderately blue, which may indicate the presence of some younger stellar populations, though the overall smooth appearance is more consistent with an older population. The galaxy exhibits a slightly elongated, but nearly circular, shape.
