This galaxy appears to be an elliptical galaxy at an approximate redshift of 0.094. The central bulge exhibits a smooth, nearly round morphology with a concentrated, yellow hue, indicative of an older stellar population. Fainter, bluer regions extend outward from the central bulge, suggesting the presence of some younger stars and possible ongoing, but likely low-level, star formation activity. There is some visible disturbance in its form, and it may be undergoing minor interaction with another galaxy. The overall structure suggests a galaxy that is transitioning from a more active state to a relatively quiescent one, with a calculated stellar mass around 10^9.9 solar masses.
