The galaxy presents as a spiral type, with a notable central bulge. The bulge appears moderately sized. The disk component is readily visible, with some indication of spiral arm structure, but this is not very prominent. The galaxy is not observed edge-on. There is no major interaction or merger event apparent. The central bulge exhibits a yellowish-orange hue, potentially indicative of an older stellar population. The disk demonstrates a bluer tint, likely due to the presence of younger, hotter stars. Overall, the galaxy displays an intermediate stage of star formation. The galaxy's morphology can be classified as a regular spiral with a dominant disk.
