The galaxy presents an overall smooth morphology, indicative of an elliptical or lenticular galaxy type. The central region exhibits a bright, concentrated bulge, suggesting a relatively high stellar density. There is a subtle color gradient observed, transitioning from a yellowish core to a redder outer halo, potentially indicative of variations in stellar populations or dust content. The galaxy appears somewhat elongated, departing from a perfectly circular shape, implying it is an intermediate elliptical galaxy or perhaps a lenticular galaxy with a faint disk. There are no prominent signs of ongoing mergers or major disturbances, although there are some faint indications of substructure within its halo. The galaxy appears to be a massive system.
