The galaxy appears to be undergoing a merger or interaction. Two distinct, roughly spherical, luminous components are visible, suggestive of two galactic nuclei in close proximity. The color of the components appears somewhat redder than the surrounding diffuse light, which implies an older stellar population or significant dust obscuration. There's some faint, irregular structure extending outwards from the central regions. Overall, the galaxy presents a disturbed morphology, not appearing as a well-defined spiral or elliptical. There may be some early signs of tidal tails, but they are not well-defined.
