The galaxy presents as a slightly inclined spiral with a relatively smooth morphology. A bright central bulge is discernible. The spiral arms appear somewhat flocculent and tightly wound, exhibiting a bluish hue suggestive of recent star formation. There is some hint of dust lanes within the disk, but the overall appearance suggests a system dominated by older stellar populations. The lack of strong, distinct features points towards a relatively undisturbed system, though minor irregularities in the arm structure hint at possible past interactions.
