The galaxy presents as a relatively smooth, elongated structure. The central bulge appears bright and yellowish, indicating an older stellar population. Moving outward from the bulge, there's a gradual transition into a fainter disk-like component, exhibiting a bluish hue suggestive of younger, hotter stars. The disk is not well-defined, lacking prominent spiral arm structure. The overall morphology leans towards a smooth, elliptical shape with a hint of a disk, although the roundness is moderate. There's no clear evidence of any major merging activity or significant tidal disturbances.
