The galaxy presents a largely smooth and rounded morphology. A bright central bulge region is visible, appearing almost spheroidal in shape. The color of the central bulge is suggestive of an older stellar population. There appears to be a disk component surrounding the bulge, with a subtle bluish hue. This suggests the presence of some ongoing star formation, though likely at a relatively low rate. There are no signs of major disturbances or tidal features, suggesting a relatively isolated evolutionary path. Overall, the galaxy appears to be a relatively undisturbed system.
