The galaxy appears to be a relatively luminous, disk-shaped system viewed at an oblique angle. Its overall color is slightly blue-green, suggesting the presence of some recent star formation. The light distribution is centrally concentrated, though not perfectly smooth. There is evidence of some structural features, possibly spiral arms, though they are not sharply defined. There appear to be some minor disturbances in the disk structure, which may be the result of a past merger. The light is dominated by a bulge, but there is also a faint disk.
