The galaxy presents as a relatively smooth, somewhat elongated structure. Its morphology is suggestive of an elliptical galaxy, possibly of type E4-E5. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is minimal evidence of spiral arms or a prominent disk component. Its color is yellowish, which could be due to older stellar populations with very little current star formation. There is a small chance this could be the result of a minor merging event, though the galaxy's form suggests it is likely an early type galaxy.
