The galaxy presents as a generally smooth, elliptical-like structure, with a high degree of central concentration. The color profile appears relatively uniform, with a slight redder hue in the central bulge. Faint disk-like features may be present, but are not easily distinguished. There is no evidence of strong spiral arm structure, the disk appears homogenous. No significant ongoing major merger events are noted. There appears to be a minor interaction or possible tidal stream feature. The galaxy appears to be relatively isolated in this field, with no close companions readily apparent. The overall morphology suggests a galaxy that has largely ceased significant star formation activity.
