The galaxy presents a generally smooth and elliptical morphology. Its color profile indicates a concentration of older stellar populations, particularly within the core. The galaxy exhibits an intermediate axial ratio, appearing neither perfectly spherical nor highly elongated. There is no discernible evidence of significant tidal disturbances, major mergers, or prominent spiral arm structures. Faint features or a subtle disk-like component cannot be entirely excluded given the image resolution, but the overall appearance suggests a quiescent system dominated by evolved stars.
