The galaxy appears as a faint, diffuse object. Morphologically, it exhibits characteristics of both smooth and featured structures. There is a subtle disk-like component, although the overall structure appears largely spheroidal. Evidence of minor disturbances is present, suggestive of a potential past interaction or minor merger. The core of the galaxy exhibits a brighter concentration of light, transitioning outwards into a more indistinct halo. There is an absence of well-defined spiral arms or a prominent bar structure. The color indices imply a relatively red galaxy, potentially indicating an older stellar population or significant dust obscuration. Overall, the galaxy is either a relatively smooth elliptical galaxy or a lenticular galaxy undergoing some form of minor interaction.
