The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness. It appears nearly circular in shape, with a subtle elongation. The light distribution suggests a concentrated central bulge that blends smoothly into the outer regions, showing a radial gradient in luminosity, decreasing from the core outwards. The color profile is predominantly yellow-orange, indicating an older stellar population likely dominated by red giant stars. The galaxy appears relatively isolated, without any prominent signs of ongoing major mergers or tidal disturbances, although subtle indications of a minor disturbance are present in the asymmetry of the outer isophotes. Evidence indicates a low star formation rate. Based on its size and luminosity, this is a moderate-mass, luminous galaxy.
