The galaxy presents an elliptical morphology. It appears relatively smooth in texture, with no readily discernible spiral arm structures or prominent dust lanes. The central region exhibits a higher concentration of light, suggesting a dense galactic nucleus. The color profile indicates a general distribution of older stellar populations, with a subtle shift toward redder hues in the core. The overall shape deviates somewhat from a perfect sphere, exhibiting a degree of flattening. There are no obvious signs of a recent major merger, though a minor disturbance cannot be ruled out at this resolution.
