The galaxy appears as a lenticular or possibly an elliptical galaxy, displaying a relatively smooth and centrally concentrated light profile. It exhibits a pronounced bulge and an extended, diffuse halo, but lacks any distinct spiral arm structure. The overall color gradient suggests a redder core and a slightly bluer halo, potentially indicating a difference in stellar populations, with older stars dominating the core and younger stars residing in the outer regions. The elongated morphology indicates that the system is not perfectly spherical, and may be subject to some tidal forces. There is no clear evidence of a major ongoing merger or significant morphological disturbance. It is likely a relatively massive galaxy with a low specific star formation rate.
