The galaxy presents as a flattened, disk-shaped system, viewed nearly edge-on. A central bulge is apparent, appearing more concentrated and yellowish. The disk itself exhibits a bluer hue, likely indicative of younger stellar populations and ongoing star formation. There appears to be some distortion and unevenness in the disk structure, possibly due to tidal interactions, but no major merger events seem to be occurring at the time of observation. The dust lane is difficult to perceive but there are some uneven dark patches along the central plane. The overall morphology is consistent with a late-type spiral galaxy, seen at high inclination.
