The galaxy appears to be a spiral galaxy, observed at an oblique angle. It presents a luminous central bulge, which is slightly elongated along the major axis of the galaxy. The bulge exhibits a yellowish hue, suggesting a population of older, cooler stars. Surrounding the bulge is a fainter, bluish disk component, indicative of younger, hotter stars and potentially ongoing star formation. The spiral arms are not well-defined, appearing somewhat flocculent and diffuse. There might be a hint of minor asymmetry or disturbance in the outer regions of the disk. The galaxy appears to have a mass of around 10^10.7 solar masses.
