The galaxy presents a smooth, largely featureless morphology. It exhibits a nearly spherical shape with a high degree of central concentration, suggesting an elliptical classification. The dominant color is a yellowish hue, indicating an older stellar population with a relative lack of ongoing star formation. There is no apparent spiral structure or significant dust lane obscuration. Faint, diffuse light extends outwards from the bright central region, but there is no evidence of tidal tails or other major disturbances indicating a recent merger. Overall, the galaxy appears as a relaxed, evolved system.
