The galaxy exhibits an elliptical morphology, appearing largely smooth in its light distribution. The galaxy presents a largely round shape, with an axial ratio close to unity. The color gradient across the galaxy indicates a redder core, transitioning to a bluer halo, suggestive of a more evolved stellar population centrally with younger, bluer stars in the outer regions. There are multiple galactic nuclei, which suggests an ongoing or recent merger. There is an additional blue source or object located towards the galactic edge. This might be a site of significant star formation activity or potentially a smaller dwarf galaxy being accreted. A minor disturbance is visible within the galaxy, likely caused by the recent or ongoing merger.
