This galaxy appears as a fairly smooth, elliptical-like object, possibly an early-type galaxy. There is a high degree of central concentration, with the light appearing most intense at the galactic nucleus and gradually fading outwards. The galaxy appears to be fairly rounded, with a slight elongation. I don't see any obvious spiral arm structures or signs of major disturbances that would indicate an ongoing merger. However, there might be a hint of some minor disturbance or interaction, as there is a slight asymmetry in the outer isophotes. The dominant color is consistent with an older stellar population, potentially indicating a galaxy where star formation is currently low. The blue hue suggests the presence of some younger, hotter stars, however the overall coloring suggests an older, redder population of stars is more dominant. Overall, it appears to be a relatively quiescent galaxy, characterized by a smooth morphology and gradual decline in brightness from the core.
