The galaxy appears to be a lenticular or possibly an elliptical galaxy, displaying a smooth, centrally concentrated light distribution. Its overall shape is elongated and oval. There's a noticeable color gradient, with a yellowish-white core transitioning to bluer hues in the outer regions. This hints at older stellar populations dominating the core while more recent star formation may be occurring in the disk. The overall morphology suggests a relatively evolved system, likely with a significant bulge component. There are faint indications of possible disturbance. Further observations are needed to confirm if this is a true merger.
