The galaxy appears to be a relatively smooth, elliptical or lenticular type system. Its light profile suggests a high degree of central concentration with a relatively gradual decrease in surface brightness outward. The color distribution is dominated by yellowish-white hues, with the central region being the brightest. The overall morphology indicates an older stellar population. The galaxy appears undisturbed, with no clear signs of tidal features, major mergers, or interactions with other galaxies. It exhibits a generally rounded shape, with no apparent distortions. There are no apparent spiral arm structures, or dust lanes present within the disk. The galaxy has a high degree of central concentration, which further supports its classification as an elliptical or lenticular galaxy with a dominant bulge.
