The galaxy presents as a cigar-shaped or elongated elliptical galaxy with a relatively smooth morphology. There is little discernible disk structure. Its color profile appears to shift from a bluer hue at the top and bottom to a more golden or reddish color towards the center. This color gradient suggests a possible variation in stellar populations, with younger, hotter stars possibly dominating the regions at the top and bottom. The central region likely contains an older, redder stellar population. There are no obvious signs of active galactic nuclei or significant dust lanes, and it appears to be relatively undisturbed, with no major merging events indicated by visual inspection. There's no indication of strong star formation from the image alone, however, its color shows signs of star formation. The galaxy appears to be an isolated system.
