The galaxy presents as a lenticular or early-type spiral, exhibiting a smooth, bulge-dominated morphology. The central bulge appears nearly spherical and is characterized by a yellowish hue, indicative of an older stellar population. A faint disk is discernible, displaying subtle spiral arm structures with hints of blue star formation regions. The outer edges of the galaxy fade gradually, suggesting a diffuse stellar halo. There are no prominent dust lanes or signs of recent major merger activity, although some minor disturbances cannot be ruled out. The overall color profile suggests that star formation is relatively quiescent compared to more active spiral galaxies.
