The galaxy presents a spiral morphology, displaying prominent spiral arms. These arms exhibit a tightly wound structure, indicative of a potentially higher shear rate within the galactic disk. The central bulge appears moderately sized, contributing substantially to the overall luminosity. A bar-like structure appears to be present but is weakly defined. The disk is not viewed edge-on. Evidence suggests ongoing or recent star formation, as indicated by the bluish hue within the spiral arms, though the overall star formation rate appears to be relatively low. There is a possible minor disturbance noted on the left side of the galaxy; possibly indicating some gravitational interaction or minor merger event.
