This galaxy presents as a largely smooth, elliptical structure. There is a bright, condensed central region, exhibiting a high degree of symmetry. Fainter, diffuse emission extends outward, gradually fading into the background. The overall shape appears to be generally round. There is very little evidence of spiral arms or distinct features, suggesting it is likely an early-type galaxy. No significant distortions are immediately apparent, implying no major merger events in its recent history. The color gradient suggests that younger stars may be present.
