The galaxy presents a somewhat smooth, disk-like structure, appearing to be relatively undisturbed. The central bulge exhibits a yellowish-red hue, possibly indicating an older stellar population. Moving outward from the bulge, a faint greenish disk is observed, suggesting the presence of younger stars and potentially some ongoing star formation. The galaxy appears moderately rounded. There is no obvious sign of a major merger or significant tidal disruption. Overall, the galaxy appears to be a relatively isolated system, exhibiting a quiescent morphology with hints of recent or ongoing star formation activity, primarily concentrated in the disk.
