The galaxy presents a morphology consistent with a spiral type, exhibiting a discernible disk structure. The spiral arms appear relatively well-defined, though somewhat flocculent in nature. The central bulge is prominent, exhibiting a color gradient that transitions from a more yellowish-orange hue in the core to a subtly bluer tone towards the outer regions of the disk. Evidence of dust lanes and star forming regions are faintly visible. The disk is oriented approximately face-on with some moderate arm winding, suggesting some amount of angular momentum. The overall structure suggests a dynamically evolved system, with the likelihood of a supermassive black hole within the galactic nucleus. Some minor interaction with other galaxies cannot be ruled out.
