The galaxy presents as a fairly smooth, elliptical structure with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, which may indicate an older stellar population. Progressing outward from the core, the color gradient shifts toward a fainter, redder tone, with a slight hint of bluer light in the outermost regions. This suggests a more complex distribution of stellar ages, with possible regions of recent or ongoing star formation within the galaxy. The galaxy appears relatively undisturbed, showing no prominent signs of tidal interactions or recent merger events. It is moderately elliptical in shape, with its major axis extending roughly across the image. Overall, the galaxy appears to be a mature, fairly massive system with a relatively high Sersic index, hinting towards a de Vaucouleurs profile.
