The galaxy presents a largely smooth, elliptical morphology. Its color profile indicates a higher concentration of older stellar populations, suggestive of a relatively low star formation rate. The galaxy displays a central bulge dominating its overall structure, with a gradual fall-off in luminosity moving outwards from the core. No significant spiral arm structures or distinct dust lanes are discernible within the image. There's a slight hint of distortion in the outer regions, which could be indicative of a past minor merger event. Overall, the galaxy appears as a mature system with minimal ongoing star formation activity and a high degree of symmetry.
