The galaxy appears to be a spiral galaxy at an approximate redshift of 0.048. It exhibits a prominent disk structure with well-defined spiral arms. The arms are tightly wound around a central bulge, suggesting a possibly older stellar population. The central bulge seems relatively small compared to the overall disk size. The bluer colors visible in the spiral arms, combined with the relatively low rate of star formation, hint at ongoing, albeit possibly subdued, star formation within the disk. There is no clear evidence of a strong bar structure, although some subtle asymmetry could indicate a weak bar. The galaxy's morphology appears relatively undisturbed, indicating no major mergers or interactions are actively occurring. There is a slight chance of a minor disturbance, but it is difficult to tell.
