The galaxy presents as an elliptical morphology, with a smooth, largely featureless appearance. The light distribution suggests a centrally concentrated bulge, characterized by a relatively high surface brightness. The outer regions exhibit a more diffuse glow, fading gradually into the background. No distinct spiral arms or bars are discernible in this observation. The overall color profile indicates a population of older stars, with a slight reddening towards the outer regions compared to the core. There's no obvious evidence of ongoing star formation activity, though some subtle color variation exists within the faint outer halo. The galaxy appears relatively undisturbed, lacking any prominent tidal features or signs of major mergers. The isophotes appear mostly regular, tending toward an elliptical shape, however, there are some very minor irregularities that suggest a small merger may have taken place.
