The galaxy presents a primarily smooth morphology, with a slightly elongated shape. The light distribution suggests a central bulge that is yellowish in color, potentially indicative of an older stellar population. Surrounding the bulge, there is evidence of a faint, bluish disk or halo, which may indicate ongoing or recent star formation. There are some subtle irregularities or disturbances apparent in the outer regions of the disk. The overall appearance suggests a galaxy that is transitioning between morphological types, potentially having undergone some minor interactions or disturbances in its past.
