The galaxy presents as a somewhat elliptical, disk-like structure with a prominent central bulge. The core exhibits a bright, yellowish-white luminosity, suggesting an older stellar population likely dominated by evolved stars. The surrounding disk shows hints of a blueish tint, potentially indicating younger star formation regions, although these features are not sharply defined. The overall smoothness of the light distribution points towards a relatively evolved galaxy, but faint disturbances cannot be ruled out in higher resolution images. No prominent spiral arm structure is visible, and there is no clear indication of an ongoing major merger event, though minor interactions are possible.
