The galaxy appears to be an elliptical galaxy, characterized by a generally smooth and featureless light distribution. It presents a concentrated central bulge that emits primarily yellow and red light. This suggests an older stellar population dominated by red giant stars. The light tapers off gradually from the core, forming a diffuse halo, which is also redder in color, further indicating that star formation is minimal or absent. The galaxy does not show any obvious signs of spiral arms, bars, or significant dust lanes, which supports its classification as an elliptical galaxy. There is no indication of recent merger activity. Overall, the morphology suggests a quiescent galaxy that has likely consumed most of its gas reserves, with only a low level of ongoing star formation.
