The galaxy presents as a centrally concentrated, yellowish-orange, smooth object. Its morphology appears largely elliptical with a high degree of circularity. There is minimal evidence of spiral arm structure or significant disk features in this image. The galaxy exhibits a relatively uniform color gradient emanating from a bright, almost stellar-like nucleus. Faint wisps of bluer light, potentially indicating areas of ongoing star formation, are subtly present in the outer regions of the galaxy, although these could also be image artifacts. The overall appearance suggests a mature galaxy with a substantial stellar mass and a low specific star formation rate, implying that star formation is not the dominant process currently taking place within the galaxy. There is no visually compelling evidence for any major or minor merging events or tidal disturbances.
