The galaxy presents as a relatively smooth, elliptical morphology. Its core appears as a bright, concentrated spheroid, exhibiting a notable luminosity. The color profile indicates a yellow-red hue, implying an older stellar population within the galaxy. There is a faint blue tinge along the outer regions. Evidence of any significant disk structure or spiral arms is absent. No major disturbances or signs of an ongoing merger are observed within the galaxy's structure, it appears to be undisturbed.