The galaxy presents a generally smooth and rounded morphology. Its light profile appears centrally concentrated, with a bright core that gradually fades into the outer regions. There is little evidence of distinct spiral arm structure or prominent features typically associated with disk galaxies. The color is consistent with a relatively old stellar population. The lack of irregularities or tidal features suggest no recent major merger events. Minor disturbances may be present but difficult to resolve. Based on the image alone, the galaxy is most likely an elliptical galaxy or a lenticular galaxy seen face-on. Its color indicates ongoing star formation, however, the overall rate seems low. The galaxy appears to be a relatively massive system.
