The galaxy appears to be a spiral galaxy viewed at a steep angle. The galaxy exhibits a bright central bulge that appears to be relatively smooth and concentrated. Extending from the bulge, a disk component is visible, showing some evidence of spiral arm structure, though it is somewhat diffuse. One side is brighter than the other, which is likely dust. The colour of the galaxy is relatively red, possibly indicating the presence of an older stellar population within the bulge, and ongoing star formation within the disk. There is faint indication of a possible minor interaction or disturbance in the disk but it might just be dust, so it warrants further investigation. The overall morphology appears to be mostly undisturbed.
