The galaxy presents a generally smooth and rounded morphology. A bright central bulge is discernible, exhibiting a yellowish-white hue, likely indicating an older stellar population. Surrounding the bulge, a fainter, more diffuse disk is observed. Hints of bluer regions are present within this disk, possibly indicating areas of more recent star formation. There is no obvious spiral structure visible, and the disk appears relatively uniform in color and brightness. The galaxy's overall shape suggests a possible transition state between a pure elliptical and a spiral galaxy. There appears to be no significant signs of interaction or tidal disturbances affecting the galaxy's morphology.
