The galaxy presents a largely smooth and centrally concentrated morphology. The light profile is consistent with an elliptical galaxy, exhibiting a radial gradient of decreasing intensity from the center outwards.  The core exhibits a yellowish hue, suggesting an older stellar population dominating the central regions.  There is a subtle color gradient visible, with the outer regions appearing slightly bluer than the core, potentially indicating a younger stellar population in those areas, or lower metallicity gas and stars.  No distinct spiral arms or dust lanes are discernible.  The overall shape appears largely spheroidal with no major mergers or obvious tidal disturbances evident in the immediate vicinity. The size is fairly compact.
