The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is broadly elliptical in shape, exhibiting a high degree of circularity. There is little evidence of spiral arms or distinct features, suggesting it may be an early-type galaxy.

The central region appears brighter and somewhat yellowish. This suggests an older stellar population dominates this region. Fainter, blueish light is visible in the outer regions of the galaxy. This hints at the potential existence of a small population of younger, hotter stars.

There is no indication of tidal tails or obvious signs of recent major mergers, though subtle distortions cannot be entirely ruled out. The galaxy does not appear to be actively undergoing a significant starburst phase.
