The galaxy appears as a centrally concentrated object with a relatively smooth and rounded morphology. It exhibits a yellowish hue, suggesting an older stellar population. There is no obvious spiral arm structure or dust lanes visible in this image. The galaxy's light profile appears to gradually fade from the core outwards. There are no visible signs of any major ongoing merger events, although a very subtle disturbance cannot be ruled out. It has an absolute magnitude indicative of a luminous galaxy. Based on its color and morphology, this galaxy is potentially an elliptical or S0 type galaxy, though greater detail is needed for definitive classification.
