The galaxy presents as a single, relatively smooth object, with no immediately apparent spiral arm structures or a distinct galactic bar. Its light is concentrated towards the center, suggesting a significant bulge component. The galaxy exhibits a subtle elongation in its overall shape, appearing somewhat elliptical rather than perfectly spherical.

There's an indication of some internal color variation. The central region exhibits a yellowish hue, potentially indicating an older stellar population or a higher dust concentration. Extending outward, the galaxy shows a slightly bluer tint, suggesting the presence of younger, hotter stars in these regions. However, these color variations are not drastic, suggesting a relatively uniform stellar population across the galaxy.

The image does not reveal any signs of ongoing major mergers or significant tidal disturbances that would indicate recent interaction with another galaxy. There appears to be no clear evidence of intense star formation regions, such as bright HII regions. This suggests a relatively quiescent state regarding star formation activity.
