The galaxy exhibits a discernible spiral structure. Arms are visible, although somewhat flocculent. The galaxy presents a distinct central bulge region. The bulge appears moderate in size relative to the overall disk. There's some visual suggestion of minor disturbances within the galaxy, possibly indicating a past or ongoing interaction with a smaller companion or the aftermath of a minor merger event. Color gradients are apparent, with bluer hues concentrated in the outer spiral arms and a shift toward redder tones in the central bulge. There is no apparent strong central bar, but we cannot rule out the possibility of a weaker bar structure that is not easily seen given this image. Given the prominence of spiral arms and the bluer colors, we can infer that the galaxy still supports star formation, but based on the color and apparent morphology, the present rate of star formation appears to be fairly subdued.
