The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, yellowish hue, suggesting an older stellar population likely dominated by evolved stars. Moving outward from the center, a subtle blueish tint becomes apparent. The overall shape is nearly circular, with no obvious distortions or tidal features indicative of a major merger event. Faint, diffuse outer regions extend outwards, indicating a halo of stars. There is no clear evidence of spiral arms or a prominent disk structure. The color profile suggests a moderate level of recent or ongoing star formation, primarily located outside the central bulge.
