The galaxy presents an elliptical morphology, appearing largely smooth and concentrated. The central region exhibits a bright, yellowish-orange hue, indicative of an older stellar population, which likely dominates the light emitted from the core. Moving outwards from the center, the color transitions to a slightly redder tone, with some subtle mottling apparent. There is a slight hint of asymmetry in the outer regions, which could be due to a minor interaction or internal disturbances, though the dominant feature is one of relative homogeneity. There is no clear evidence of distinct spiral arms or a prominent disk structure. Overall, the galaxy's light profile suggests a relatively quiescent state, with limited ongoing star formation.
