The galaxy appears to be a relatively smooth, centrally concentrated system. The light distribution suggests an elliptical morphology, appearing largely spheroidal with a high degree of roundness. There is no strong evidence of spiral arms or a prominent disk structure. The galaxy exhibits a bright, yellowish core which fades gradually into its outer regions, indicating a possible older stellar population. There is very little evidence of significant tidal disturbances or ongoing merger activity. The light is consistent with a system where star formation is suppressed relative to the overall stellar mass.
