The galaxy presents a largely smooth morphology with a central concentration of light that gradually decreases outwards. The overall shape appears elliptical, tending towards an intermediate roundness rather than a highly elongated or perfectly spherical form. There is a notable absence of distinct spiral arms or other prominent features indicative of disk structures. The color profile suggests a population of older stars, indicated by its yellow hue and reduced star formation rate. There is no evidence of major mergers or significant tidal disturbances in its immediate vicinity. Minor disturbances may be present but not easily visible.
