The object presents as a disk galaxy, viewed at a high inclination, nearing edge-on. A central bulge is visible, appearing somewhat bright and concentrated. Faint spiral arm structures, primarily on one side are present, displaying clumpy regions which might indicate areas of ongoing star formation. There's a possible distortion in the overall shape, hinting at a gravitational interaction or merger event in the relatively recent past. The dust lane is evident along the galaxy’s mid-plane, absorbing and reddening light from stars behind it. The color profile suggests a mix of stellar populations, with bluer hues in the outer regions of the disk.
