The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. It exhibits a slight elongation, presenting a shape that is close to round. The galaxy's color profile suggests a relatively evolved stellar population, dominated by older, redder stars. There is a lack of distinct spiral arm structure or prominent dust lanes, supporting its classification as an elliptical galaxy. The lack of irregular features suggests that the galaxy is not currently undergoing any major merger events or tidal interactions. Overall, the galaxy appears to be a typical elliptical system, characterized by its smooth light distribution and lack of significant ongoing star formation.
