The galaxy presents as a flattened, disk-like structure, oriented approximately horizontally in the image. The central region exhibits a concentrated, bright nucleus appearing yellow in color. Fainter, blue-tinged, diffuse light extends above and below the central region, suggesting the presence of spiral arms or a more extended disk component. The galaxy appears relatively undisturbed, with no clear evidence of ongoing major mergers or tidal features. The overall color gradient suggests the possibility of ongoing star formation in the outer regions, which is possibly bluer, while the yellow central region could indicate an older stellar population. The object is of moderate angular size, but this is relative to the image scale and cannot determine the actual size without further data.
