This appears to be a spiral galaxy with a prominent central bulge exhibiting a yellowish hue, indicative of an older stellar population. The spiral arms are tightly wound, and clearly defined, extending outwards from the bulge, displaying a bluish tint, implying the presence of ongoing star formation within these regions. There seems to be a clear, defined disk extending from the center, viewed at a non-edge-on angle. The lack of distinct dust lanes suggests a relatively face-on orientation, and the observed light suggests a modest amount of obscuring dust. There may be a slight asymmetry present, possibly indicating past or ongoing interactions with another galaxy. There is no evidence of a strong bar-like structure.
