The galaxy presents as a system with a dominant, relatively smooth bulge. This central region exhibits a yellow-white hue, suggesting an older stellar population. The galaxy appears to have a flattened disk component, extending outwards from the bulge. There's a slight hint of bluer color within the disk, indicating the presence of younger, hotter stars and regions of ongoing star formation, although at a low rate. The overall morphology suggests a galaxy that is largely undisturbed, although there are some subtle irregularities visible at the disk’s edge that could indicate minor tidal interactions or disturbances. The object is neither perfectly round nor elongated, appearing as an intermediate shape. There is no strong evidence of a major merger event.
