The galaxy presents a predominantly smooth, elliptical morphology. Its color profile appears consistent, with a yellowish-orange hue concentrated towards the central region, suggesting an older stellar population with reduced ongoing star formation. There is a slight elongation, deviating somewhat from a perfectly circular form, with no discernable spiral arm structures. The galaxy exhibits a high degree of central concentration, with light intensity diminishing gradually towards the outer edges. No significant signs of tidal disturbances or ongoing major mergers are visible, with the overall structure appearing relaxed and undisturbed.
