The galaxy presents as a lenticular, disk-shaped system with a noticeable central bulge. The bulge exhibits a smooth, concentrated luminosity profile, transitioning into a less luminous, more diffuse disk. There is faint evidence of a ring or arm-like feature extending from the disk, appearing as a slight color differentiation within the galaxy. No obvious spiral arm structure is visible. The galaxy does not present a disturbed or asymmetric morphology, lacking indications of recent major mergers or interactions. The light distribution suggests that the older stellar population dominates the galactic system. The elongation of the galaxy suggests some degree of rotation and flattening. The galaxy is approximately 4.7 kpc across. The galaxy exhibits a redshift, indicating that it is moving away from us.
