The galaxy appears to be a disk-shaped object, viewed at a relatively high inclination. Its central bulge is prominent and displays a smooth, concentrated distribution of light, appearing almost spherical. The disk component exhibits a more diffuse and fainter light distribution compared to the bulge. I observe a slight bluer tinge to the galaxy suggesting ongoing star formation within its structure, particularly in the outer regions of the disk. There is a general smoothness to the light profile. Although the galaxy appears mostly undisturbed, there are slight asymmetries within the disk, suggesting potential minor interactions or disturbances within its recent history, it looks slightly warped. Overall, the galaxy seems to be an intermediate spiral or lenticular type galaxy.