The galaxy appears to be relatively compact in size, exhibiting a somewhat amorphous morphology. The central region of the galaxy is notably bright and concentrated, suggesting a dense population of stars or a potentially active galactic nucleus. Moving outward from the center, the intensity of light decreases. 

There is a subtle asymmetry in the outer regions of the galaxy, potentially indicative of gravitational interaction or a past merger event. A slight tidal tail might be forming, but it is hard to be sure. No definitive spiral arm structure is visible within the resolution of the image. The color profile of the galaxy transitions from a blue-white core to a more yellow and red outer edge. The red is subtle, however. 
