The galaxy presents a largely smooth and elliptical morphology. It appears predominantly round in shape, with a slight deviation towards an intermediate form. The central region exhibits a concentrated luminosity profile, suggesting a high stellar density. There is a noticeable color gradient from the core outward. The core appears to be a yellowish-orange hue, suggesting an older stellar population, while the outer regions show a subtle shift toward redder tones. There is no discernible spiral structure or prominent disk component. There are no significant signs of tidal disturbances, major mergers, or ongoing interactions with neighboring galaxies. The overall appearance suggests an evolved system with relatively low star formation activity.
