The galaxy presents as a smooth, elliptical morphology with a high degree of central concentration. The core is a bright, intensely luminous region, exhibiting a yellow hue. The isophotes appear elongated, with a cigar-shaped form factor. There's little evidence of defined spiral arms or prominent dust lanes. The outer regions show a gradual decrease in luminosity without clear structural features such as rings or distinct shells. The overall impression is that of a relatively undisturbed, evolved galaxy, lacking significant ongoing star formation. Faint distortions are possibly visible, but not conclusive enough to be considered significant. No obvious signs of a major merger event are apparent, and the galaxy appears largely isolated.
