The galaxy presents as a somewhat elliptical structure, appearing mostly smooth in texture. There's a bright central bulge that dominates the light emission, suggesting a high concentration of stars in the galactic nucleus. The galaxy exhibits a yellowish hue, especially concentrated in the central bulge. A slight disc-like structure can be inferred by the galaxy's subtle elongation, though distinct spiral arms are not visible. There are some indications of minor disturbances in the outer regions. The overall morphology indicates that the galaxy is likely an early-type spiral or potentially a lenticular galaxy transitioning from a spiral to an elliptical form.
