The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge that emits strongly in the yellow-red wavelengths, suggesting an older stellar population. The outer regions diffuse gradually, with decreasing light intensity. The morphology is largely undisturbed, showing no prominent tidal features or signs of recent major mergers. The elongated shape indicates some level of asymmetry, though the overall structure is primarily smooth. It's stellar formation rate is very low.
