The galaxy presents a generally elliptical morphology. A bright, concentrated central bulge is apparent, exhibiting a cyan hue, possibly indicative of active star formation or a strong emission line contribution. The surrounding galactic disk appears relatively smooth, lacking distinct spiral arm structures. There is a subtle gradient in color and intensity from the center outwards, with the outer regions exhibiting a dimmer, slightly redder tone suggesting an older stellar population. Some irregularities are present in the outer regions of the galaxy disk, which could potentially suggest past interactions or minor disturbances. There is no evidence of a major ongoing merger. The galaxy lacks strong features, suggesting an earlier morphological type, such as an S0 or early-type spiral.
