The galaxy presents as a somewhat elongated, elliptical structure. Its central region appears to be dominated by older stellar populations, exhibiting a yellowish-orange hue, indicative of a lack of recent star formation in this area. Moving outwards from the core, the color shifts slightly, becoming a bit bluer. This suggests the presence of younger, hotter stars within the galaxy's outer regions. However, compared to typical spiral galaxies, star formation activity seems relatively subdued, with a moderate rate indicated by its color gradients. The galaxy's light profile appears smooth, with no obvious signs of spiral arms or a prominent disk component. This supports its classification as an elliptical or lenticular galaxy. The object also displays an intact morphology, with no strong indications of recent or ongoing major mergers. Though it displays no obvious distortions to its shape, a minor disturbance or interaction in the past cannot be ruled out.
