This galaxy presents as an edge-on disk galaxy. A prominent central bulge is observed, appearing somewhat rounded and elongated along the disk. The disk appears relatively thin and shows some subtle color variations, potentially indicating differential dust extinction or regions of varying stellar populations within the plane. Overall color is consistent with an older stellar population, as there appears to be not very much blue star formation. However, there are small areas that might indicate the presence of active regions of star formation. There is no evidence of a recent major merger or significant tidal disturbances in its morphology. There may be a slight asymmetry, suggesting a minor interaction or internal dynamics affecting the galaxy's structure. The galaxy is relatively smooth and appears to be quite distant.
