The galaxy appears as a relatively compact object, exhibiting a roughly elliptical morphology. There is a dominant central bulge with a high degree of symmetry. The galaxy displays a mixture of colors, with a particularly bright, almost cyan/white core, suggesting a concentration of younger, hotter stars or a possible active galactic nucleus. The surrounding disk presents a gradient of color, with an inner region that appears to be green or blue. This suggests a possible spiral arm structure with associated ongoing star formation. Patches of red can be seen on the perimeter of the galaxy. Overall, the galaxy gives the impression of being relatively smooth, with no clear indications of major ongoing mergers or tidal disturbances.
