The galaxy presents as a relatively smooth, elliptical structure with a centrally concentrated luminosity profile. The core appears bright and yellowish, suggesting a population of older stars. There is a gradual decrease in surface brightness extending outwards from the core. The overall color appears redder in the outer regions compared to the core, possibly indicating a change in stellar population or dust content. The galaxy does not exhibit any clear spiral arm structure or significant dust lanes. There are no obvious signs of major tidal disturbances or ongoing mergers, with the galaxy exhibiting a largely undisturbed morphology. The elongation of the galaxy suggests an intermediate ellipticity.
