The galaxy presents as a somewhat elongated, disk-like structure viewed at an oblique angle. Its central region exhibits a concentrated brightness, appearing nearly smooth and spheroid in form, colored in a yellow-orange hue, indicative of an older stellar population dominating the core. A less intense blue-greenish color is visible throughout the galaxy's disk, surrounding the central bulge. There are subtle hints of spiral arm structure within this outer region, but it is not sharply defined. The overall morphology suggests a later-type spiral galaxy with a dominant bulge component and ongoing, yet potentially subdued, star formation. There are no obvious signs of recent major mergers or significant tidal disturbances to the galaxy's structure.
