The galaxy presents as a largely smooth, elliptical object with a concentration of luminosity towards the center. Its color profile exhibits a warm, reddish-yellow hue, suggestive of an older stellar population. There is a slight elongation, but the galaxy appears primarily round, although some intermediate shapelessness is also apparent. No prominent spiral arm structures or significant dust lanes are discernible. The galaxy seems isolated, with no obvious signs of ongoing major mergers or tidal disturbances from nearby galaxies, although minor disturbances or past merger events cannot be ruled out at this resolution. The overall appearance is consistent with that of a relatively massive elliptical galaxy exhibiting low to moderate star formation rates.
