The galaxy presents as a mostly smooth, elliptical-like structure with a concentrated central bulge. A slight elongation is observed, suggesting a departure from perfect circularity. Color gradients indicate the presence of a relatively old stellar population, with a more pronounced concentration of redder hues toward the galactic center. There is no discernible evidence of active star formation regions or prominent spiral arm structures. The overall morphology suggests a dynamically relaxed system, potentially resulting from past merger events.
