The galaxy presents as a system of multiple interacting galaxies. The dominant galaxy appears as a relatively smooth elliptical structure with a bright, concentrated core. Fainter, more diffuse light extends outwards, forming an irregular halo around the central region.

There are nearby galactic structures indicating an ongoing interaction, with visible tidal features suggesting gravitational disturbances. The color profile indicates a dominance of older stellar populations, with a relatively low rate of star formation. The galaxy exhibits a moderate mass, based on its luminosity and morphology. The system demonstrates signs of past or current merging events, with possible minor disturbances in its structure.
