The galaxy presents a largely smooth, elliptical morphology. The color distribution indicates a central concentration of older stellar populations, exhibiting a reddish hue, surrounded by a more extended region with a greenish tint, suggesting the presence of younger stars or ionized gas. No distinct spiral arms or bar structures are discernible. The galaxy displays a moderate ellipticity, appearing somewhat flattened. There are no clear signs of ongoing major mergers or significant tidal disturbances in its immediate vicinity, although subtle asymmetries could indicate minor interactions in the past. Overall, the galaxy appears to be an evolved system, likely a massive elliptical with a relatively low rate of current star formation.
