The galaxy presents as a face-on spiral, exhibiting a prominent central bulge. The bulge appears yellowish in color, suggesting an older stellar population. Spiral arms are clearly visible, extending outwards from the central bulge. These arms appear somewhat loosely wound, indicating a possibly later-type spiral galaxy. The spiral arms display a bluer hue, which may correspond to regions of active star formation. The disk appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There is a suggestion of a possible bar structure crossing the central region of the galaxy, and dust lanes are visible within the disk. The galaxy demonstrates a moderate size and an apparently high luminosity.
