The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with brightness decreasing steadily outwards from a bright, compact core. The overall shape is nearly round, with minimal deviation from circularity. The galaxy appears to be relatively undisturbed, lacking any obvious signs of tidal interactions, mergers, or significant morphological distortions. There is subtle color variation, with a slightly bluer hue observed in the outer regions, possibly indicating ongoing, though modest, star formation activity within those areas, as compared to the core which appears more yellow or red. The galaxy does not show any prominent spiral arms or a distinct disk structure.