The galaxy presents as an elliptical or lenticular type, exhibiting a centrally concentrated bulge with a gradual decrease in luminosity outward. The primary color appears to be a yellow/white hue, suggestive of an older stellar population. There is evidence of a faint, blue-ish extended disk with low surface brightness, potentially indicating some star formation activity. There is also what may be a small tidal tail or merger remnant on one side of the galaxy. Overall, the system shows indications of being relatively evolved.
