The galaxy presents an overall elliptical morphology, exhibiting a smooth, diffuse light distribution with a high degree of central concentration. The light profile appears predominantly uniform, lacking distinct spiral arm structures or significant dust lane obscuration. There is a slight elongation, deviating marginally from a perfectly circular shape, and it is considered a "in between" round shape. No evidence of major ongoing mergers or significant tidal disturbances is discernible, although the possibility of minor interactions cannot be entirely ruled out. The galaxy's color profile indicates a relatively evolved stellar population, with a moderate red color suggesting a lower rate of active star formation.
