This galaxy appears to be a relatively luminous and massive system observed at a redshift of approximately 0.14. The galaxy exhibits a prolate spheroid shape, appearing elongated or cigar-shaped. A significant portion of the galaxy's light is concentrated in a smooth, centrally located bulge, which displays a yellowish-orange hue suggesting an older stellar population. Fainter disk-like component showing some blueish tinges surrounds the bulge, indicating a younger stellar population and ongoing or recent star formation, particularly at its periphery. There appears to be some minor disruption or interaction occurring in the system, hinting at a past or ongoing minor merger event. Overall, the galaxy presents a morphology consistent with an intermediate stage of galaxy evolution, possibly transitioning from a disk-dominated spiral to an elliptical-like system.
