The galaxy presents as a relatively smooth, elliptical structure. Its light is dominated by a central reddish core, which suggests an older stellar population. The outer regions show a transition to a greenish hue, which may indicate the presence of a younger stellar population and/or ongoing star formation, though the colors could also represent redshift effects. The galaxy appears moderately inclined to our line of sight. There are no obvious signs of strong spiral arms or a significant disk component. The overall morphology suggests a galaxy undergoing or having completed a transition from active star formation to a more quiescent state.
