The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology with a high degree of central concentration. The light profile is relatively uniform, lacking any distinct spiral arm structures or prominent dust lanes. It is very round, showing minimal elongation and no indication of tidal disturbances or recent merger activity. Color gradients within the galaxy are subtle, transitioning from a yellowish core to slightly redder outer regions. This may indicate an older stellar population and lower levels of ongoing star formation. The size suggests a relatively massive galaxy. Overall, the galaxy presents a well-defined, symmetrical shape consistent with a dynamically relaxed system.
