The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. The core is a bright, almost uniform, yellowish-white, suggesting a large population of older stars. The overall shape appears relatively round, lacking any prominent features such as spiral arms or a distinct disk structure. The color gradients suggest a slightly bluer halo, possibly indicating some younger stellar populations at the periphery, though the galaxy appears relatively quiescent in terms of star formation. There is no visual evidence of ongoing mergers or significant tidal disturbances.
