The galaxy presents as a relatively smooth, centrally concentrated structure. Its shape is elongated, appearing somewhat cigar-shaped with a high fraction of in between roundness. The light profile suggests a dominant bulge component, exhibiting a concentrated core. There is a hint of a disk component present, with some bluer regions potentially indicating areas of ongoing star formation, though the overall star formation rate appears to be low. The central bulge appears yellowish. The overall structure indicates the galaxy has not experienced any major mergers or significant disturbances recently. It appears to be undisturbed. The galaxy’s color suggests an intermediate population mix, without a strong preference toward blue, young stars or red, old stars.
