The galaxy presents as a fairly well-defined spiral, although the spiral arms appear somewhat flocculent. A significant portion of the galaxy's light is concentrated in a central bulge, which appears relatively smooth and featureless. The disk component is prominent, exhibiting a mixture of bluer and redder hues, potentially indicating varying stellar populations.  There's a slight indication of minor disturbance within the disk structure, potentially hinting at past interactions or internal dynamics. The galaxy is neither a pure elliptical nor a strongly interacting system, showing a degree of structural integrity with the noted disk and spiral characteristics. The galaxy's overall color is moderately red, possibly indicative of a moderate amount of dust obscuration.
