The galaxy appears as a moderately luminous, elliptical system. Its color indices suggest a dominant population of older stars, giving it a yellow-orange hue. The galaxy exhibits a degree of elongation, appearing more cigar-shaped than perfectly spherical. While the majority of its light appears smooth and centrally concentrated, there is subtle visual evidence suggestive of minor tidal disturbances, which could indicate past or ongoing interaction with another galaxy, though the structure itself is still largely undisturbed. There is no clear evidence of active star formation or pronounced spiral arms within the visible light spectrum. Overall, the galaxy presents as a mature, relatively quiescent system.
