The galaxy appears as a somewhat diffuse, moderately bright object with a suggestion of a disk-like structure. Its overall color is bluish, indicating the presence of younger, hotter stars, possibly associated with on-going or recent star formation. There is a slightly brighter central region, which may indicate the presence of a galactic bulge. Faint, disturbed features can be vaguely perceived in the disk which may point to past or ongoing gravitational interactions or merger activity. Overall, the galaxy presents a mixed morphology, showing properties between an elliptical and a spiral. The estimated size seems to be of an average galaxy.
