The galaxy appears to be a relatively compact object, with a centrally concentrated light profile. Its overall shape is elliptical, exhibiting a fairly smooth and regular structure with only minimal signs of significant disturbance. The core of the galaxy is a bright and concentrated, with colors trending towards bluer wavelengths. This suggests a possible population of younger, hotter stars concentrated within the galactic nucleus, or it might be a signature of the presences of an active galactic nuclei. The outer regions of the galaxy transition to redder hues, indicating a potentially older stellar population or a higher concentration of dust. There are no prominent spiral arms or bar structures visible, suggesting that the galaxy is most likely a elliptical galaxy. Overall, the galaxy appears to be isolated, showing no clear signs of major merger activity or significant tidal interactions.
