The galaxy exhibits a generally smooth morphology, but also displays some indications of disturbed features. There is evidence of a central bulge, exhibiting a reddish hue, potentially indicating an older stellar population. Surrounding this bulge is a more diffuse, bluish region, suggestive of ongoing or recent star formation. There is a slight asymmetry to the galaxy's overall shape, and some disturbances that may be the result of either a minor or major disturbance. The galaxy is more disc-like than perfectly round, but more round than cigar-shaped. It could possibly be undergoing or have undergone merging activity.
