The galaxy presents as a face-on spiral, exhibiting prominent spiral arm structures. These arms appear to be well-defined, with a flocculent morphology. The color distribution suggests active star formation within the spiral arms, indicated by bluer hues, which contrasts with the yellower, redder bulge. The bulge region appears relatively small, though its color suggests an older stellar population. The disk of the galaxy appears nearly circular. There is no visual evidence of a strong central bar structure, or major ongoing merger activity. There are no apparent signs of tidal tails or other significant disturbances.
