The galaxy appears as an elliptical-shaped object, exhibiting a generally smooth morphology. The central region displays a yellowish hue, which may indicate an older stellar population dominating the core. Moving outwards from the center, the color gradually shifts towards a bluer tone, potentially indicating a younger stellar population or the presence of ongoing star formation within the outer regions. The overall structure lacks prominent spiral arms or other distinct features, which supports its classification as an elliptical galaxy. There appears to be some minor irregularity, but no major disturbances detected.
