The galaxy presents as a smooth, elliptical morphology with a high degree of central concentration. The core region exhibits a significantly higher luminosity compared to the outer regions, appearing almost stellar. The ellipticity is notable, presenting a cigar-like shape. There's little evidence of spiral arm structure or prominent dust lanes. Faint blue tinges along the edges may indicate some star formation. The absence of significant distortions suggests it is undisturbed, without apparent ongoing major mergers or tidal interactions. 
