This galaxy exhibits a generally elliptical morphology, appearing somewhat elongated. The light distribution is relatively smooth and concentrated towards the center. A bulge component appears prominent, displaying a yellowish hue, likely indicative of an older stellar population. The outer regions of the galaxy exhibit a more diffuse, bluish color, possibly suggesting the presence of younger, bluer stars or ongoing star formation within a disk-like structure. There is no visual evidence of strong spiral arm structures or major mergers, although subtle disturbances might be present in the outer regions. The overall structure suggests a galaxy transitioning towards an elliptical morphology, possibly a lenticular galaxy.
