The galaxy exhibits a generally smooth morphology, with no clear spiral arm structure or pronounced features immediately apparent. Its overall shape appears elliptical, though it leans slightly toward a more rounded appearance than a highly elongated one. The central region displays a higher concentration of light, suggesting a prominent galactic nucleus. The galaxy's color profile indicates an older stellar population, shifting toward the redder end of the spectrum. There is no obvious evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's structure.
