The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a prominent, relatively bright central bulge. This bulge appears to be composed of older stellar populations, indicated by its yellowish hue. A faint, somewhat indistinct disk surrounds the bulge. The disk component demonstrates a bluer color, suggesting ongoing or recent star formation, albeit at a modest rate. The galaxy has a moderately inclined orientation with respect to our line of sight, giving it an elliptical appearance. There is little to no evidence of strong spiral arm structure or significant dust lanes. Overall, the galaxy seems relatively smooth and undisturbed.
