The galaxy presents a generally smooth morphology, with a high degree of roundness. There is no apparent spiral structure or distinct disk. The primary color is a yellowish-orange hue, suggesting an older stellar population and lower levels of ongoing star formation. Faint extensions of light are visible surrounding the central region, implying a diffuse halo or extended stellar distribution. There appears to be only a slight, if any, disturbances to the galaxy’s structure based on the high degree of smoothness observed, which likely indicates the galaxy has not experienced any major recent merger events. The overall appearance is consistent with an elliptical galaxy at a considerable distance, where detailed structural features are not easily resolved.
