This galaxy presents as a spiral galaxy, observed at an angle close to face-on. There is evidence of spiral arm structure extending from the central bulge region. These arms show noticeable star forming regions within the disk, exhibiting a bluer hue, indicative of younger, hotter stars. The central bulge presents a more yellow/red appearance, suggesting an older stellar population. While the bulge is not completely obscured by dust, there is a moderate amount of dust present within the galaxy disk, as well as possible indication of HII emissions. There are no obvious signs of tidal disturbances or interactions with other galaxies, suggesting that this galaxy is relatively undisturbed. There does not appear to be a prominent bar structure.
