The observed galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellow-orange hue, indicative of an older stellar population. The disk component is faint but discernable, appearing elongated with hints of bluer regions possibly indicating ongoing, although relatively low, star formation. The overall structure suggests a galaxy in a later stage of its evolution, displaying minimal signs of recent major merger events, although potentially experiencing minor gravitational interactions given the subtle disturbances in the outer regions. The galaxy presents a shape that falls between a completely round and elongated form.
