The galaxy presents an elongated, somewhat elliptical morphology. A bright, concentrated central bulge appears yellowish-white in color, suggesting an older stellar population in the core. The outer regions of the galaxy exhibit a fainter, bluer hue, indicating the presence of younger stars and potential ongoing star formation. The galaxy is observed nearly edge-on, with a disk-like structure apparent, though without clearly defined spiral arms. There is a subtle dust lane bisecting the galaxy. The overall structure suggests an intermediate-type spiral or lenticular galaxy, showing a mix of bulge and disk characteristics.
