The galaxy appears to be a disk galaxy, relatively face-on. It exhibits a bright, concentrated central bulge. The disk component is clearly visible, with hints of spiral arm structure. The colour suggests that it is made up of old stars and is not forming many new stars. The smooth appearance of the galaxy suggests that it is not undergoing any major mergers or interactions with other galaxies. There is some evidence of minor disturbances in the galactic disk. Overall, this galaxy seems to be a settled system, with a stable disk and bulge. The size is typical for a galaxy of its kind.