The galaxy presents as an elliptical morphology with a high degree of central concentration. The light profile appears smooth, lacking distinct spiral arm features or significant dust lane obscuration. A color gradient is discernible, with the core exhibiting a more yellow-gold hue that transitions to a redder color in the outer regions. No signs of tidal tails or shell structures are observed, suggesting relative dynamical quiescence. The isophotes appear largely regular and elliptical, indicative of a well-relaxed system with a large population of older stars. Faint irregular extensions of the galaxy seem to exist on the edges of the disk.
