The galaxy presents as a centrally concentrated object with an elliptical morphology. The light distribution appears generally smooth, lacking prominent spiral arm structures or strong irregularities. The central region displays a warmer color, suggestive of an older stellar population or dust obscuration, while the outer regions show bluer hues, hinting at the presence of younger stars. The overall shape deviates slightly from perfectly round, exhibiting a somewhat elongated, cigar-like appearance. There are no obvious signs of ongoing major mergers or tidal disturbances, although minor interactions or subtle disturbances cannot be entirely ruled out based on this image alone.
