The galaxy presents a smooth, elliptical morphology. The core exhibits a high degree of luminosity, suggesting a concentrated stellar population, potentially an active galactic nucleus. The galaxy shows a radial color gradient, transitioning from a yellowish-white center to a slightly redder outer halo. This could indicate an aging stellar population in the outer regions. The galaxy appears to be relatively undisturbed, with no signs of major mergers or tidal distortions. It appears to be a relatively isolated system. The overall shape is primarily spheroidal with only a slight deviation towards a cigar shape.
