The galaxy presents as a centrally concentrated object. Its overall morphology appears elliptical, with a relatively smooth, featureless structure. The core region exhibits a high degree of luminosity, suggesting a significant concentration of stars. The light profile gradually diminishes from the center outwards, with no apparent spiral arms or distinct morphological features beyond the core. The galaxy displays a subtle color gradient, with a slightly bluer hue in the outer regions compared to the more neutral-colored core, possibly indicating ongoing star formation at a low rate. There is no obvious evidence of significant tidal interactions or ongoing mergers. The galaxy's shape is moderately rounded, without any prominent elongation.
