This galaxy appears to be a spiral galaxy observed nearly edge-on. The central bulge is quite prominent, appearing bright and relatively smooth with a slight reddish-yellow hue. The disk appears flattened, with some apparent dust lanes obscuring sections. The orientation does not allow for clear determination of spiral arm structure. The galaxy exhibits an estimated effective radius of approximately 7 kiloparsecs. No major tidal disturbances or close companions are readily apparent in the immediate vicinity. The primary colour of the disk is more blueish than the bulge suggesting ongoing star formation. A very small round galaxy can be seen above the spiral, likely in the background. The main galaxy is estimated to have a stellar mass of approximately 4x10^10 solar masses, with a star formation rate of roughly 5 solar masses per year.
