This galaxy presents as an elliptical or lenticular type. It exhibits a smooth, concentrated light profile with a dominant central bulge. The galaxy appears elongated, with a moderate ellipticity. A slight color gradient is visible, transitioning from a yellowish-white core to a bluer, fainter outer halo. There is no discernible spiral arm structure or significant dust lane obscuration. No obvious signs of recent major merger activity are observed, such as tidal tails or strong morphological distortions, though subtle disturbances may be present. Based on its morphology and color, this galaxy is likely a relatively massive system with a substantial population of older stars and a low rate of ongoing star formation.
