The galaxy appears to be a spheroid-shaped system with a relatively smooth light distribution, showing only minor hints of features. It has a notable central concentration of light, appearing brightest towards the core with intensity diminishing outwards. The overall color profile indicates a redder hue. There is an orange blob beside it, possible another galaxy or part of the initial galaxy. Based on these characteristics, a likely classification would be an elliptical galaxy with potentially ongoing, but not intense, star formation activity. There is no obvious sign of significant disturbances due to any current major merging events. The general appearance suggests a morphologically evolved galaxy.
