The galaxy presents as a moderately luminous, early-type system exhibiting a smooth, elliptical morphology. The central region displays a concentrated, bright core, transitioning into a diffuse halo. The color profile shows a general trend of redder hues in the core, indicative of an older stellar population, with a subtle bluer shift outwards into the halo suggesting a younger, possibly ongoing, star formation. The galaxy appears undisturbed with no visible signs of major mergers or tidal interactions. Its overall shape is neither perfectly spherical nor significantly elongated, presenting an intermediate ellipticity. 
