The galaxy exhibits a complex morphology, appearing as a potential interacting system. One component presents a relatively smooth, elliptical profile with a concentrated core, suggesting an older stellar population and minimal ongoing star formation within this region. The second component displays a disk-like structure, inclined relative to our line of sight. This component shows a bluer hue, possibly indicative of younger, hotter stars and active star forming regions. The overall appearance is "in between" round and cigar-shaped, with a possible minor disturbance to its structure. The system has a considerable size and a red shift measured around 0.11.