The galaxy presents a generally elliptical morphology. The central region exhibits a concentration of light with a yellowish hue, likely indicating an older stellar population. Moving outwards from the core, the light gradually diminishes in intensity, showing a transition towards bluer colors. This suggests the presence of younger, hotter stars in the outer regions, though these features are subtle. Overall, the galaxy appears relatively smooth in texture, with no obvious signs of strong spiral arms or active star formation regions. There is also a slight elongation to its shape, with no significant disturbances or signs of recent mergers.
