The galaxy presents a relatively smooth and symmetrical morphology. The light is concentrated in the center. The galaxy exhibits a color gradient, transitioning from a yellowish hue at the core to a faint blue tinge in the outer regions. This color variation may indicate a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outskirts. The observed light distribution suggests the galaxy is dominated by a spheroidal component. There is no obvious spiral structure. There is no signs of active galactic nuclei activity from what is observed.
