The galaxy presents a disk-like morphology, viewed nearly edge-on. There is evidence of internal structure, possibly spiral arm features, though the resolution is limiting. The galaxy exhibits a color gradient, appearing bluer towards the extremities and redder toward the central bulge. This suggests ongoing star formation in the outer regions. Dust lanes appear to bisect the disk. The overall impression is of a relatively massive disk galaxy with a moderate star formation rate. There may be a slight disturbance in the disk's symmetry, indicating a potential past or ongoing minor interaction with another galaxy.
