The galaxy presents as an elongated structure, with a central bulge that appears relatively smooth in texture. There's an indication of a disk component, but it is poorly defined and appears somewhat disturbed or disrupted. The color distribution suggests an older stellar population throughout the galaxy, with perhaps a few regions of bluer, younger stars in the outer areas, and more prominently in a singular region along the elongated major axis. There's a noticeable difference in the color and luminosity along the galaxy, indicating possible ongoing interactions or mergers with another system or tidal disturbances. The overall structure is not perfectly symmetrical, suggesting that it might not be a relaxed, isolated system. The profile appears to be relatively concentrated, hinting towards a significant spheroidal component.
