This galaxy exhibits a spiral structure with prominent arms emanating from a central bulge. The bulge appears moderately sized, transitioning smoothly into the disk. The spiral arms are well-defined and appear to be undergoing active star formation, indicated by their bluer hue. There is a noticeable asymmetry in the arm structure and some disturbances in the morphology, which may be indicative of tidal interactions with a smaller nearby galaxy or recent merger event. There appears to be a faint bar-like structure bisecting the bulge. The disk is not viewed edge-on; its orientation provides a relatively face-on view of the spiral structure. The overall color suggests a mix of stellar populations, with regions of younger, bluer stars in the spiral arms and older, redder stars concentrated in the bulge.
