The galaxy presents a slightly inclined disk morphology. The central bulge appears prominent and exhibits a smooth, yellowish-orange color, suggesting an older stellar population. The disk component shows bluer regions indicative of ongoing star formation, although these are not distinctly resolved into individual star-forming regions. The overall structure suggests a possible spiral or lenticular galaxy, with hints of faint spiral arm structure. There appears to be some minor disturbance in the disk, as it looks asymmetric. The galaxy exhibits a moderate degree of concentration of light towards the center.
