The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Coloration suggests a mix of stellar populations, with a central region exhibiting a yellowish-white hue, indicative of older stars. The outer regions transition to a slightly more blueish-white color, hinting at the presence of younger, hotter stars. While the overall structure is smooth, there may be subtle features within the disk indicating ongoing processes. There do not seem to be any major disturbances in the image.
