The galaxy appears to be a spiral galaxy, viewed at a moderate inclination. There is evidence of distinct spiral arms, tightly wound around a central bulge. The bulge exhibits a moderate size relative to the overall disk. The galaxy displays a smooth, but not perfectly elliptical shape, suggesting a disk-like structure. Faint color gradients are observed within the galaxy, trending towards bluer hues in the outer disk, potentially indicative of ongoing star formation. The core appears more yellow, possibly indicative of older stellar populations. There is no obvious sign of major disturbances or a significant ongoing merger event. A possible weak bar structure might be present. The overall light distribution is relatively concentrated.
