The galaxy presents as a single, relatively symmetrical object. Its overall shape approximates an ellipse, exhibiting a significant degree of roundness. The central region is characterized by a high concentration of light, appearing as a bright, yellowish core that gradually fades towards the outer edges. This central region suggests an older stellar population. The galaxy's color profile transitions from yellowish in the center to a more bluish hue in the outer regions, suggesting possible ongoing star formation, albeit at a low rate. There is no clear evidence of spiral arm structures or a distinct disk component. The galaxy appears relatively smooth in texture, with no obvious signs of major disturbances, tidal tails, or merging activity. Overall, it exhibits properties consistent with an elliptical galaxy possessing some characteristics of a transitioning or quiescent system.
