The galaxy presents as a relatively smooth object, with a slight elongation. It appears to be a single, unified body, lacking distinct spiral arms or a prominent bar structure. The color profile suggests a mix of stellar populations, with a centrally concentrated yellowish-white hue, possibly indicating an older population of stars. The outer regions appear slightly redder, which may indicate regions of dust extinction or older star formation. There is no strong evidence of active star formation regions. Overall, the galaxy exhibits characteristics consistent with an elliptical galaxy, although it could possibly be a lenticular type seen face-on. Further spectroscopic analysis would be needed to determine its exact composition and properties, as well as its inclination, and assess if recent or ongoing interactions may be impacting its form.
