The galaxy presents as a relatively smooth, elliptical form with a high degree of central concentration. Its color gradient suggests an older stellar population, with the core exhibiting a yellowish-orange hue, potentially indicating a population of evolved stars. The outer regions of the galaxy appear to fade gradually, without sharp edges or distinct spiral arm structures. There is a subtle flattening observed, deviating slightly from a perfectly spherical shape towards a more lenticular morphology. Indications suggest it might be a lenticular galaxy due to the lack of spiral structure. There are no obvious signs of active star formation regions. No significant tidal tails or distortions are apparent, suggesting a lack of recent major merger events.
