The galaxy presents as a moderately luminous, elongated system. It appears to be an edge-on or nearly edge-on spiral or lenticular galaxy. The central bulge exhibits a yellowish hue, suggesting an older stellar population and a relative lack of ongoing star formation within this region. The disk appears relatively smooth, with a faint bluish tint. The pronounced color difference from the bulge implies the presence of younger, bluer stars. The galaxy shows no evidence of strong tidal features or major disturbances that would indicate recent major merger events. The galaxy exhibits a slight color gradient, with the central bulge being redder and the outer disk becoming bluer.
