The galaxy presents as a disk-shaped system, viewed at a moderately high inclination. There is a distinct central bulge, appearing as a bright, concentrated region. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the bulge, the galactic disk displays a bluish tint, indicative of ongoing star formation and the presence of younger, hotter stars. The disk is relatively smooth in appearance with faint indications of spiral arm structure. The galaxy's overall morphology appears undisturbed, with no obvious signs of major mergers or tidal interactions, although there may be a minor disturbance. The galaxy appears somewhat elongated, deviating slightly from a perfect circular shape, with an overall size which may be approximately 4 kiloparsecs in radius.
