The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a central concentration of light, appearing brightest in the core, which gradually diminishes outwards. The galaxy appears elongated, with a moderate ellipticity. The primary color is a yellowish-white hue, indicative of an older stellar population. Fainter, diffuse extensions are observed beyond the main body of the galaxy but remain indistinct. No clear spiral arm structures or dust lanes are visible. There is no sign of major tidal disturbance, such as distorted structure or extended plumes. The color suggests a relatively low ongoing star formation rate. The light profile suggests that the galaxy is of substantial mass.
