The galaxy appears as a slightly elongated, diffuse object with a smooth light distribution. The dominant color is a yellowish-white, possibly indicating an older stellar population. There is little evidence of strong spiral arm structure or prominent dust lanes. A slight deviation from perfect roundness is observed, which could be due to a minor interaction or internal dynamics. No obvious merging features are detected. The overall morphology suggests an elliptical galaxy or a lenticular galaxy viewed at a relatively face-on angle. The lack of blue color further suggests relatively low current star formation activity.
