The galaxy appears to be a spiral or lenticular type, seen at an oblique angle. There is a central bulge that appears bright and somewhat yellow-orange in color, indicative of an older stellar population. Fainter, bluer light extends outwards from the bulge, suggestive of younger stars and star-forming regions within the galaxy's disk. Some irregularities are visible in the outer regions, potentially signifying minor disturbances or interactions with other galaxies. The galaxy is more elongated than circular.
