The galaxy appears as a smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually diffuses outwards. The color profile suggests a dominant population of older stars, with a yellowish-orange hue concentrated in the core region. There's a subtle transition towards redder tones in the outer regions. No distinct spiral arms or dust lanes are discernible. The galaxy's overall shape indicates a system that is neither perfectly spherical nor highly elongated, exhibiting characteristics in between these shapes. There is little indication of any major ongoing merging activity or significant tidal disturbances, although there is a hint of a possible minor disturbance.
