The galaxy presents a generally smooth, elliptical morphology. The light distribution indicates a high degree of central concentration with a gradual decrease in surface brightness towards the outer regions. There is a subtle color gradient visible, exhibiting a slightly bluer hue towards the outer edges in comparison to the more yellow-white core. This could suggest the presence of younger stellar populations in the outskirts. There is no strong evidence of spiral arm structures or a prominent disk. Faint disturbances are visible in the galaxy. The galaxy appears relatively isolated with no apparent signs of recent major merger events.
