The galaxy presents as an intermediate spiral with a relatively bright nucleus. One arm appears well-defined, exhibiting a yellow-orange hue, indicative of an older stellar population. The other arm appears somewhat more disturbed or diffuse, showing a bluer component, suggesting more recent star formation. The disk of the galaxy appears asymmetric, with the brighter arm being longer and more extended. The morphology of the galaxy is somewhere between round and cigar-shaped. No significant merger activity is apparent, though there is evidence of minor gravitational disturbances. Overall, the galaxy demonstrates a combination of evolved stellar populations and ongoing star formation within its disk.
