The object presents as a spiral galaxy with a prominent central bulge. The bulge exhibits a smooth, concentrated luminosity profile. The surrounding disk component appears somewhat elongated. Faint spiral arms can be discerned, exhibiting a moderately wound structure. The orientation of the galaxy is slightly tilted relative to our line of sight. The central region displays a yellowish hue, indicative of an older stellar population, while the outer disk shows hints of bluer colors. Some dust lanes might be obscuring parts of the disk, but more detailed inspection would be required to confirm this. There do not seem to be any obvious signs of interaction or recent major merger events impacting its overall structure. Overall the galaxy appears to be a relatively undisturbed spiral galaxy.