The galaxy presents as a centrally concentrated spheroid with a smooth overall appearance. There is a slight elongation visible, indicating a possible deviation from a perfectly circular shape. A dominant yellowish-white color is present at the core, suggestive of an older stellar population. Fainter, diffuse bluish hues surround the core, potentially indicating regions of younger stars or ongoing, though subdued, star formation. No prominent spiral arm structures or dust lanes are discernible, suggesting a more evolved morphological type. There are no signs of any major interaction with other galaxies. Overall, the galaxy appears as a relatively quiescent system, with a large mass and a fairly low star formation rate.
