The galaxy appears to be an elliptical galaxy with a relatively smooth, symmetrical morphology. It presents as a concentrated, centrally bright object, with a diffuse halo suggesting older stellar populations. The color indices suggest a redder overall hue, consistent with an evolved stellar population and a likely low current star formation rate. There is no obvious spiral structure or ongoing major mergers distorting its shape. The galaxy exhibits a generally rounded form with a minor asymmetry; there is no definitive cigar-shaped profile or merging activity. The overall impression is that of a passively evolving, relatively undisturbed system.
