The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. Its shape appears largely rounded, with only a slight elongation visible. The color profile exhibits a central concentration of yellow light, indicative of an older stellar population dominating the core. There is a subtle disk-like structure. Though a small percentage of features are suggestive of a merger, the overall symmetry of the galaxy and the relative lack of significant tidal tails or distortions would suggest that it is a relatively relaxed system and that if a merger did occur, it was likely some time ago. A low rate of star formation, with high mass in comparison to the rate.