The galaxy presents a primarily smooth morphology, with a concentrated central bulge that exhibits a yellowish-orange hue. This central region is suggestive of an older stellar population. Fainter, more diffuse extensions emanate from the core, creating a halo-like appearance. These outer regions appear less structured and bluer in color, perhaps indicating more recent star formation activity. There are some subtle hints of disturbed features, but overall the galaxy appears relatively undisturbed.
