The galaxy presents as a luminous, elliptical-like structure with a smooth, featureless appearance. The central region exhibits a concentrated, bright core that gradually diffuses outward. The overall color appears to be a yellowish-white hue, potentially indicating an older stellar population. There is a slight elongation, but it is difficult to assess the exact axis ratio from this image. No prominent spiral arms or distinct dust lanes are discernible. The morphology suggests a galaxy undergoing little to no active star formation and no ongoing merging activity. There is a general lack of blue light indicating low levels of star formation.
