The galaxy presents as a somewhat elliptical structure with a smooth, diffuse appearance. The central region displays a concentration of light, appearing brighter and more yellow in color, suggesting an older stellar population. Moving outwards from the core, the color gradually shifts toward the redder end of the spectrum, possibly indicating the presence of dust or older stars. There is a subtle hint of a disk-like structure, though the galaxy is largely spheroid in shape. No distinct spiral arms or other features are readily apparent. The galaxy does not show signs of any major disturbances and appears to be isolated.
