The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually fades into its outer regions, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The color profile suggests a predominantly older stellar population, with a yellow/red hue dominating the central and inner regions. There is little evidence of significant dust lanes or regions of active star formation in the image. The overall morphology indicates a mature galaxy, likely an elliptical or lenticular type, undergoing minimal current star formation activity.
