The galaxy presents as a relatively smooth, disk-shaped structure. A central bulge is evident, exhibiting a yellow-white hue suggestive of an older stellar population. The surrounding disk appears bluer, hinting at ongoing or recent star formation. The galaxy's form is more lenticular than spiral, and shows hints of a smooth dust lane. The system does not display any obvious signs of major merger activity, though a faint asymmetrical extension on one side could indicate a minor interaction or tidal feature.
