The galaxy presents a primarily smooth morphology. It exhibits a generally round shape, with a minor deviation toward an intermediate ellipticity. There is no strong evidence of major disturbances or ongoing mergers in this image, although some minor asymmetric features are present which could point towards a slight gravitational interaction. The galaxy's light profile shows a concentrated bulge with a gradual falloff in surface brightness moving outward. Color gradients suggest a relatively homogeneous stellar population within the galaxy, with a slight trend towards redder colors in the central regions, hinting at an older stellar population within the bulge. The blue light emanating is from the disk. The overall appearance suggests an evolved system.
