The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The core exhibits a bright, yellowish hue, indicating a population of older stars. Fainter, bluer regions are observed in the outer regions of the galaxy, suggesting the presence of some younger stellar populations. The galaxy shows a slight elongation in its shape. There are no immediately obvious signs of a major ongoing merger, although subtle asymmetries could indicate minor gravitational interactions or past merger events. There are no obvious spiral arms, or strong dust lanes. The galaxy exhibits moderate redshift, suggesting a considerable distance. Based on its overall appearance and color, it appears to be an early-type galaxy, possibly an elliptical or lenticular galaxy, with a relatively low rate of star formation.
