The galaxy presents a complex morphology, exhibiting characteristics that suggest both smooth and disk-like structures. The central region displays a concentrated, smooth component, likely indicative of an older stellar population or a bulge.  However, a fainter, more extended structure surrounds this core, possibly indicating a disk or spiral arms. There appears to be a region of more intense, bluer light.

Furthermore, morphological analysis suggests interaction or merger activity. While a dominant component suggests no ongoing major merger event, there is evidence of minor disturbances and possible tidal features or asymmetries in the outer regions. These features imply the galaxy may have undergone a minor merger or gravitational interaction with another galaxy in the past.
