The galaxy presents a complex morphological structure, suggestive of an ongoing or recent interaction. Two distinct components are visible, exhibiting differing color profiles. The northern component appears as a relatively smooth, concentrated spheroid, characterized by a blue-white hue. This color may indicate a younger stellar population or significant ongoing star formation within this region. 

The southern component displays a more diffuse structure and exhibits a yellowish-red color, hinting at an older stellar population or the presence of significant dust obscuration. Evident are faint tidal features extending from the main body of the galaxy, which may represent the remnants of a disrupted galactic structure or material stripped from the galaxy during an interaction. There may also be a faint plume of stars leading from one object to the other. The overall shape of the galaxy is irregular.
