This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The core region presents a bright, yellowish hue, suggesting a population of older stars. Moving outward from the core, the galactic disk appears less defined, transitioning to a blueish color, potentially indicative of younger stellar populations within the outer regions. While no prominent spiral arm structures are apparent, there are suggestions of minor asymmetries or disturbances in the disk. There is no indication of any ongoing major merger event or significant tidal disruption. The galaxy displays a near-circular shape.
