The galaxy appears as a single, centrally condensed object. It exhibits a smooth morphology, lacking any discernible spiral arms or a distinct disk structure. The light distribution is relatively even across the galaxy, with a slightly more concentrated central region. Its shape is generally round, although with a subtle elongation. There is no visible evidence of recent or ongoing merger activity or major tidal disturbances. The galaxy's color is skewed towards the redder end of the spectrum, suggesting an older stellar population and a lower rate of star formation. Overall, the galaxy presents a fairly quiescent appearance, consistent with an elliptical or lenticular classification.
