The galaxy presents a largely smooth, elliptical morphology. It is generally round in appearance, though with a slight elongation. The light distribution suggests a concentration of older stellar populations, inferred from the redder hue, especially towards the core. There's little discernible evidence of significant spiral arm structure or active star formation regions within the observed wavelengths, although lower-level activity cannot be ruled out. No major tidal features or morphological disturbances indicative of a recent major merger are apparent; however, some degree of minor interaction or disturbance is not excluded based on the subtle irregularities in its shape and light distribution. The galaxy appears relatively isolated.
