The galaxy presents as a lenticular or early-type spiral morphology. The central bulge appears large and relatively smooth, with a yellowish hue, potentially indicating an older stellar population. There is faint evidence of a disk structure. Faint spiral arms may be present, though their morphology is not well-defined. Overall the galaxy appears relatively undisturbed with only minor signs of any recent merger activity, if any. The galaxy's integrated color suggests that there is a relatively low current star formation rate and a moderate stellar mass. The overall shape is mostly rounded in appearance, with a slight deviation from perfect circularity. 
