The galaxy presents a smooth, elliptical morphology. Its light profile is concentrated toward the center, indicative of an older stellar population dominating the core. The galaxy exhibits a slight elongation, appearing more oblate than spherical. The color appears to be a pale yellow-white, suggesting a lack of significant ongoing star formation. There is no evidence of spiral arms or a prominent disk structure, and no indications of major mergers or tidal disturbances. The light distribution appears relatively uniform, with a smooth gradient from the central bulge outwards. Faint hints of bluer regions at the periphery might indicate trace amounts of younger stars, although this could be attributed to background noise. Overall, the galaxy appears to be a relatively evolved, quiescent system.
