The galaxy presents a lenticular morphology, exhibiting a smooth, elliptical shape with a noticeable central bulge. The bulge appears yellowish-white in color, suggesting an older stellar population. The disk surrounding the bulge displays a fainter, somewhat bluer hue with what looks like traces of spiral structure, hinting at the presence of younger stars and regions of active star formation. The disk appears significantly elongated, with an aspect ratio suggesting it is viewed at a substantial inclination. There is little evidence of major disturbances or ongoing merger activity. The galaxy appears relatively isolated, with no close companions immediately visible.
