The galaxy presents as a somewhat elongated, lenticular-like structure. A concentrated, bright central bulge dominates the galaxy's luminosity. Extending outward from the bulge, a fainter disk is observed. The disk appears relatively smooth with hints of some diffuse spiral structure, though no distinct, well-defined arms are apparent. One end of the disk has a faint reddish glow, which could potentially indicate ongoing star formation. The overall color suggests an older stellar population. There is no apparent significant tidal distortion or other major disturbance indicative of a recent major merger, but a minor irregularity cannot be ruled out. The general morphology suggests a galaxy in transition.
