The galaxy presents as a relatively smooth, elliptical structure, characterized by a bright, concentrated central bulge. The light profile appears to fade gradually from the core, suggesting a diffuse stellar halo. There is a slight elongation, with a generally oval shape, neither perfectly spherical nor highly flattened. No distinct spiral arms or prominent dust lanes are discernible. A hint of bluer hues is visible, potentially indicating some degree of ongoing star formation. There appear to be no signs of major mergers or significant tidal disturbances.
