The galaxy presents a disk-like morphology, viewed at a significant inclination. The disk exhibits a prominent dust lane along its major axis, obscuring light from the galactic bulge. A possible tidal tail can be seen indicating a previous or ongoing merger. The main body of the galaxy is relatively smooth, with a diffuse light distribution that suggests a relatively low star formation rate. The color appears slightly bluer in the disk than in the bulge region, hinting at a younger stellar population there. There also seems to be a second galactic body to the side, although it might be a galactic structure.
