The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing nearly spherical and luminous. The light gradually decreases with radial distance from the core, with a transition to a fainter, more diffuse outer region. There is a subtle elongation that suggests the galaxy is not perfectly spherical, leaning toward an intermediate shape. No distinct spiral arm structures or prominent dust lanes are readily apparent. The color profile appears relatively uniform, suggesting a largely older stellar population with minimal ongoing star formation. There are no indications of a major merger event or significant tidal disturbances in its immediate vicinity.
