The galaxy presents a generally smooth morphology, with an apparent lack of distinct spiral arms or a prominent bar structure. The light distribution suggests a concentration of luminosity toward the galactic center, with a gradual decrease in surface brightness at larger radii. The overall shape appears somewhat elliptical, deviating slightly from a perfect circle. A subtle extension or tidal feature might be present on one side, hinting at possible interactions or past mergers. The color profile indicates a population of older stars, as inferred from the reddish hue in the galaxy's central regions, gradually transitioning to slightly bluer colors in the outer areas. There may be moderate star formation activity. Overall, the galaxy seems to be a large elliptical galaxy at a considerable distance.
