The galaxy appears to be a relatively compact elliptical galaxy, exhibiting a smooth, concentrated light profile. Its overall shape is generally elliptical, but closer to an in-between elliptical, with no obvious disk-like structure or spiral arms visible. The core region displays a bright, centrally concentrated luminosity, suggesting a high density of stars within that region.

The galaxy's color indices suggest a population dominated by older stars, evidenced by its moderately red appearance. While the galaxy's color suggests the presence of a population of older stars, there is still some bluer light present, hinting at the presence of some recent, yet low, level of star formation. There are no signs of tidal tails, strong distortions, or other significant disturbances in the galaxy's structure, suggesting it hasn't undergone any major merger events recently. Overall, the galaxy presents a relatively undisturbed morphology.
