The galaxy presents as a smooth, elliptical form with a notable concentration of luminosity towards its center. A distinct color gradient is visible; the core exhibits a yellowish-white hue, potentially indicating an older stellar population. Fainter, bluish tones are observed at the periphery, suggesting the presence of younger stars or regions of ongoing star formation, albeit at a low rate. The overall shape leans towards a slightly elongated, cigar-like appearance. There is no obvious evidence of ongoing merging activity or major disturbances, although subtle asymmetries might indicate minor past interactions.
