The galaxy presents as a moderately bright, face-on spiral galaxy with a central bulge and discernible spiral arm structure. The core region exhibits a yellowish hue, suggesting an older stellar population. The spiral arms appear somewhat diffuse, displaying a bluer color indicative of ongoing star formation. Some minor disturbances may be present in the outer regions of the disk. The estimated stellar mass is substantial. Observed star formation rate suggests the galaxy is actively forming stars but at a moderate rate.