This galaxy presents as a relatively small, edge-on spiral. There is a subtle but noticeable central bulge. Faint disk structures extend outwards, being more diffuse on either side. A dust lane is faintly visible bisecting the galaxy along its major axis, obscuring some of the light from the bulge. There are indications of patchy star formation regions within the disk, appearing as subtle variations in color and brightness. Overall, the galaxy appears to be relatively smooth and undisturbed, showing no significant signs of tidal interactions or major mergers. The light appears to be dominantly redder in the central regions, suggesting an older stellar population, while the disk exhibits bluer hues indicative of ongoing or recent star formation.
