The galaxy presents a largely smooth morphology, with a concentrated central bulge. There is little evidence of spiral arm structure or distinct features; it appears lenticular, possibly an elliptical galaxy. Color gradients indicate a potential aging stellar population. The core is a warm yellowish white, likely indicating a population of older, lower-mass stars. Fainter blue regions exist in the galactic disc, potentially indicating current star formation. The lack of a prominent disk suggests that star formation rates are minimal. The galaxy shows no indication of a major merger or significant disturbances. The shape appears nearly circular.
