The galaxy presents as a disk galaxy, observed at a slight angle relative to face-on. Spiral arm structures are clearly visible, exhibiting a relatively tightly wound morphology. A central bulge component is present, although it appears small relative to the disk. Star formation seems to be occurring within the spiral arms, as indicated by a mottled texture. The colouration suggests a range of stellar populations, with bluer regions likely indicating recent star formation and older populations present in the less distinct regions. There is no apparent ongoing major merger activity, and the galaxy generally appears as an isolated system. The galaxy displays notable disk structures and overall shape despite the small bulge.
