The galaxy presents as a roughly elliptical or spheroidal structure, appearing largely smooth in texture with a high degree of central concentration. The core region exhibits a bright, yellowish hue, possibly indicating an older stellar population or significant dust obscuration of bluer light. Moving outward from the core, the galaxy's color transitions to a more reddish tone, suggesting a similar aged stellar population in the outer regions. Faint, diffuse outer regions are slightly oblong, displaying little evidence of spiral arms or significant disk features. There might be some slight disturbances along the edges, however, these are not pronounced. The structure presents minimal signs of recent or ongoing major merger activity.
