The galaxy presents as a centrally concentrated, relatively smooth system with a roughly elliptical morphology. The primary color of the galaxy appears to be a yellowish-white, suggesting a dominant population of older stars. The lack of strong blue colors indicates a relatively low current star formation rate. Faint reddish regions are observed, indicating the presence of possible recent star formation. The morphology is not indicative of a strong disk structure or spiral arms. The smoothness and roundness suggest it may be an early-type galaxy, possibly an elliptical or lenticular galaxy. There is possible evidence of some minor disturbances nearby to the main body of the galaxy that could be merger remnants.
