The galaxy presents a disk-like morphology with a noticeable central bulge. The bulge appears moderately sized and exhibits a yellowish hue, suggesting an older stellar population. Surrounding the bulge, a faint spiral structure can be discerned. The spiral arms are not tightly wound, and appear somewhat patchy with regions of blue indicating ongoing star formation. Some areas appear to have dust lanes within the spiral structure. The overall structure suggests that this galaxy is not undergoing a major merger, but some minor gravitational disturbance may be present. The galaxy is inclined with respect to our line of sight, but is not edge-on.
