The galaxy presents as a relatively smooth, elliptical morphology. There is little to no discernible disk structure or spiral arm presence. The core is a bright yellow-ish white, with a gradual decrease in intensity towards the edges, forming a halo. The galaxy appears somewhat compact. There is no apparent active galactic nuclei or significant dust lane obscuration. The light distribution suggests an evolved stellar population, with a higher concentration of older stars. There are no obvious signs of tidal disturbances or ongoing mergers, though very subtle minor interactions cannot be ruled out. The overall shape is not perfectly spherical, trending towards slightly elongated but not cigar-shaped. 
