The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall color profile suggests a population of older stars, contributing to a yellowish-red hue concentrated toward the center. The outer regions exhibit a more subdued blue tint, possibly indicating a small amount of younger, bluer stars are populating the outskirts. The galaxy's shape is mostly rounded, with no immediately apparent spiral arm structures or significant tidal disturbances. There's an indication of minimal ongoing star formation activity due to the lack of bright blue star-forming regions and its smooth texture. It is likely a passively evolving system with a substantial stellar mass. There might be some dust absorption within the galaxy.
