The galaxy presents as a highly inclined disk galaxy, appearing nearly edge-on from our line of sight. The central bulge is prominent and appears largely smooth and somewhat rounded. A relatively thin disk extends outwards from the bulge, with a discernible change in color from the center to the outer regions, possibly indicating differing stellar populations or dust lane obscuration. There is no visually detectable bar structure. The morphology appears relatively undisturbed, with no signs of ongoing major merger activity or significant tidal distortions. Overall, it appears to be a fairly well-ordered system, with a clear disk component. Based on the estimated luminosity and star formation rate, the galaxy appears to be actively forming stars.