The galaxy presents as a largely smooth, elliptical structure. There is a concentrated central bulge which appears slightly yellow/orange in color, suggesting an older stellar population. The overall morphology exhibits a high degree of roundness. There is no prominent disk or spiral arm structure visible. A very slight asymmetry in the outer regions may indicate a past minor interaction or disturbance, but no significant merger activity is apparent. The galaxy's color indices suggest a lack of active star formation within the galaxy. The galaxy appears to have a high mass.
