The object presents as an elliptical galaxy with a smooth, diffuse light distribution, displaying a cigar-like shape. The central region exhibits a slightly brighter, concentrated core that fades gradually into the outer regions of the galaxy. There is a distinct lack of discernible spiral arm structures or prominent dust lanes. Overall, the galaxy's morphology suggests a classification toward the elliptical end of the Hubble sequence, potentially an E4-E7 type, and the color appears to be more red than blue, indicating an older stellar population. The object does not exhibit any signs of ongoing merger activity or significant tidal disturbances.
