The galaxy exhibits a predominantly smooth morphology, with a relatively high degree of central concentration. The overall shape is elliptical, approaching circular, with minimal visual evidence of spiral arms or a distinct disk structure. The galaxy appears to be relatively undisturbed, showing no significant signs of ongoing or recent major mergers or tidal interactions. Color gradients suggest a generally evolved stellar population, with bluer colors in the central regions, likely due to the presence of younger stars or ongoing low-level star formation. The galaxy's radial light profile suggests a relatively high Sersic index, indicating a departure from a simple exponential or Gaussian profile, consistent with a more concentrated light distribution.
