The galaxy appears to be a spiral galaxy observed edge-on. There is a prominent central bulge with a somewhat rounded morphology. The disk is clearly visible, displaying a relatively smooth texture without apparent strong spiral arm features. The disk shows a blueish tint with an apparent indication of relatively active star formation on one end. The overall light distribution suggests that the bulge dominates the galaxy's luminosity, gradually fading towards the disk. No strong signs of ongoing major mergers are discernible, though minor disturbances might be present.
