The galaxy presents a complex morphology, suggesting a possible interaction or merger event. A central, relatively bright core exhibits a yellowish hue, indicative of an older stellar population. A diffuse, extended halo surrounds this core, appearing smoother and less structured. There is evidence of a faint, distorted arm or tidal tail extending from the galaxy, further supporting the hypothesis of gravitational interaction. The overall shape is neither perfectly elliptical nor spiral, hinting at a disturbed morphology resulting from the aforementioned interaction. Star formation appears to be minimal within the central region, but may be present within the distorted outer regions. The galaxy exhibits an intermediate redshift, classifying it as relatively distant. The lack of a well-defined disk structure and the presence of tidal features suggests that this system is undergoing a morphological transformation.
