The galaxy exhibits a generally smooth morphology, with a discernible disk-like structure oriented at an oblique angle to the line of sight. The central region is characterized by a bright, concentrated bulge component showing a yellowish hue, indicating an older stellar population. The disk appears slightly elongated, deviating from a perfectly circular form towards a more cigar shaped form. The outer regions of the disk display a bluer color gradient. There is no obvious evidence of strong spiral arm structure or major merger events. Faint asymmetries or minor disturbances cannot be completely ruled out. The overall appearance suggests a galaxy that is relatively evolved with a notable spheroidal component.
