The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. The color profile suggests an older stellar population, dominated by redder wavelengths. There is very little visual evidence of spiral arms or dust lanes. The overall shape is quite round, displaying minimal elongation or asymmetry. No indications of active galactic nuclei are directly apparent from the image. The galaxy exhibits a high degree of smoothness, suggesting a lack of recent major merger events. Overall, it appears to be a quiescent galaxy with a substantial mass and low rate of star formation.
