The galaxy presents as a somewhat irregular, disk-like structure. The central region exhibits a concentrated, bright core, suggestive of a bulge component. Moving outward from the center, the disk displays a mottled texture with hints of spiral arm structures, though these are not sharply defined. The galaxy's light is predominantly bluish-white, implying a significant population of young, hot stars, and possibly ongoing star formation. The overall shape is neither perfectly circular nor highly elongated, appearing somewhere in between. There is some evidence of minor disturbances in the outer regions of the disk, possibly indicative of past or ongoing interactions. A faint reddish area appears on the lower edge of the galaxy. 
