The galaxy presents a morphology consistent with an elliptical type, exhibiting a smooth, concentrated light profile. The galaxy appears to be relatively face-on, displaying a flattened spheroidal shape. The color gradient suggests an older stellar population dominating the core, which appears more yellow. Fainter, bluer regions seem present on opposite sides of the core, possibly indicating faint dust lanes or regions of more recent, albeit minimal, star formation. There is evidence of a faint and diffuse halo surrounding the central body of the galaxy. The structure indicates a galaxy that has likely undergone significant merging activity in its past, leading to the observed smoothed morphology.