The galaxy presents as a somewhat elliptical structure, displaying a relatively smooth overall appearance. The central region exhibits a pronounced concentration of light, suggesting a dense stellar population or active galactic nucleus. Moving outward from the core, the light intensity gradually diminishes, forming a diffuse halo. While a distinct disk structure is not readily apparent, subtle asymmetries hint at potential underlying features or minor disturbances. There may also be small merging events, but it appears that the galaxy is not heavily disturbed. There is a hint of color variation within the galaxy, with the central regions displaying slightly yellower hues compared to the outer regions, suggesting potential differences in stellar populations or dust content.
