The galaxy appears to be an elliptical galaxy, or possibly a lenticular galaxy viewed at a significant inclination. The galaxy exhibits a centrally concentrated bulge that transitions smoothly into a fainter, elongated disk or envelope. The color profile is predominantly reddish-yellow in the central region, suggesting an older stellar population and lower rates of current star formation within the nucleus. The outer regions show a slight bluer tint, indicating the presence of at least some younger stars. There is no visual evidence of strong spiral arms or active star-forming regions. The overall morphology is smooth, with little to no apparent dust lanes or significant irregularities. There is no evidence of tidal tails or major merger events. The galaxy displays an apparent axis ratio suggesting it is not viewed face-on, and shows an apparent axis ratio indicating an elliptical shape.
