The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. Its overall color profile shifts from a redder hue towards the center to bluer tones in the outer regions. This may indicate an older stellar population concentrated in the galactic core, with younger, bluer stars populating the periphery. There is a hint of disk-like structure, although the galaxy is largely spheroidal, without distinct spiral arms or a pronounced central bar. Some minor disturbances, such as tidal tails, are visible in the outer halo of the galaxy, but a major merger does not appear to be occurring. The galaxy is also exhibiting some star formation, which may be causing the blue color observed in the outer regions. The light is not uniform across the galaxy, but generally smooth.
