The galaxy presents a generally elliptical morphology, appearing as a smooth, concentrated light distribution. There is a bright, central core, possibly indicative of an active galactic nucleus or a high density of stars in the galactic bulge. The outer regions show a gradual decrease in luminosity, extending further along a preferential axis suggesting a slightly flattened shape. Color gradients within the galaxy appear minimal, with a subtle blue shift towards the center, which could indicate a population of younger, hotter stars. The lack of prominent spiral arms or dust lanes suggests this galaxy is likely an early-type galaxy, possibly an elliptical or lenticular galaxy. There are no obvious signs of ongoing major mergers or strong tidal interactions.
