The galaxy presents a largely smooth, elliptical morphology. The color profile shows a strong central concentration of light, appearing yellowish-orange, indicative of an older stellar population. The galaxy exhibits a high degree of roundness. There is no evidence of spiral arm structure, bars, or significant dust lanes. The galaxy shows no signs of recent or ongoing major merger activity. Minor disturbances cannot be ruled out, but there are no clear tidal features, plumes, or disrupted morphologies present in the image. The overall impression is that of a relatively relaxed and evolved system.
