The galaxy presents as an elliptical or lenticular system, appearing mostly smooth with little discernible internal structure. Its morphology is predominantly spheroidal, displaying a high degree of central concentration. There is a bright central bulge, possibly indicative of a supermassive black hole residing at the galaxy's core. The light distribution is elongated and somewhat cigar-shaped. Faint blue tinges are visible, perhaps indicating some active regions of star formation, albeit likely at a low rate. There is no visual evidence of ongoing major mergers or tidal disturbances. The system is relatively isolated in the image.