The galaxy presents a morphology consistent with an early-type spiral or lenticular galaxy. There appears to be a bright, somewhat diffuse central bulge exhibiting a yellowish hue. Faint, disk-like features extend outwards, though the arms lack distinct definition and appear flocculent. A subtle blue tint is visible within the outer regions of the disk, potentially indicative of recent star formation, albeit at a low rate. No prominent dust lanes or ongoing major merging activity is apparent. The overall structure suggests a system that is relatively undisturbed, possibly transitioning toward a more quiescent state in its evolutionary history. There is evidence of only minor gravitational disturbances.
