The galaxy presents as a somewhat elongated, diffuse object. A central bulge is apparent, exhibiting a yellowish-orange hue, suggesting a population of older stars. The outer regions display a bluer color, which could indicate more recent star formation, albeit at a low rate. The galaxy's overall structure is relatively smooth, though some subtle irregularities are visible in the disk, possibly suggestive of minor gravitational disturbances. There isn't any large scale signs of merging visible in the image.
