The galaxy presents a generally smooth, elliptical appearance with a discernible disk-like structure. The central region exhibits a bright, moderately concentrated bulge. Proceeding outward, the galaxy shows a gradient decrease in luminosity. The colors across the galaxy appear to be somewhat uniform, although some bluer regions are visibly apparent, suggestive of star formation. The morphology suggests a system that is not undergoing any major merging events, showing only mild disturbances. The galaxy has a relatively high degree of roundness. Based on the observed colors and structure, the stellar population within the galaxy appears to be a mix of older and younger stars.
