The galaxy presents as a relatively compact and luminous object. Its morphology appears largely elliptical with a high degree of central concentration. There is no discernible spiral arm structure. The galaxy exhibits a smooth, rounded profile. There is no indication of any major merger events or tidal disturbances. Color gradients indicate a generally older stellar population. The galaxy displays a slight yellowish hue at its core, which transitions to a redder color further out. This suggests a decline in star formation activity and a greater presence of older, redder stars in the outer regions.
