The galaxy presents as a luminous entity, approximately circular in projection, with a relatively smooth overall morphology. There is a clear concentration of light towards the center of the galaxy, suggesting a bulge component. While the image quality limits detailed analysis, there appears to be some degree of structure within the galaxy, hinting at the presence of faint arms or disk-like features. The color gradient transitions from a yellowish-white core to bluer outer regions. This color variation could indicate ongoing star formation in the outer parts. Given the smooth appearance, the galaxy is likely an early-type spiral or a lenticular galaxy with characteristics suggesting modest star formation. The outer edges of the galaxy appear somewhat disturbed, possibly due to minor gravitational interactions or mergers with smaller galaxies.
