The galaxy presents a moderately elliptical morphology with a central bulge that appears quite smooth and dominant. There is evidence of ongoing or recent interaction or merger activity. The galaxy exhibits distinct color variations across its structure. The core region displays a yellowish hue suggesting an older stellar population, whereas a region of bluer color is offset from this core, implying a younger stellar population in this area. This could be indicative of tidal features or star formation triggered by a past gravitational interaction. The overall structure of the system is not clearly defined with no distinct spiral arms. The galaxy exhibits a moderately bright profile, suggesting significant stellar mass. Based on its appearance, the galaxy is likely undergoing a transformative period, either from merging or strong internal processes that significantly affect its morphology and stellar populations.
