The galaxy appears to be a spiral galaxy viewed at a slight angle. There is a central bulge that emits a yellowish light, suggesting an older stellar population. The bulge transitions into a disk component, where a hint of spiral arm structure is visible, though somewhat faint and possibly tightly wound. The galaxy exhibits a relatively smooth overall appearance, but there are some indications of possible disturbances or minor mergers, potentially causing some asymmetry in the disk. The estimated size of the galaxy is a few kiloparsecs across, fairly typical for spiral galaxies. The presence of the disk indicates ongoing or recent star formation.
