The galaxy appears to be a relatively smooth, elliptical galaxy with a slightly elongated shape, possibly classified as E4 or E5 on the Hubble sequence. Its light distribution suggests a dominant bulge component, with a smooth transition in brightness from the core outwards. The central region exhibits a yellowish hue, potentially indicative of an older stellar population. There is a lack of prominent spiral arm structures or significant dust lanes, which supports the classification of an elliptical galaxy. No signs of major mergers or tidal disturbances are clearly visible in this image, though a slight asymmetry cannot be ruled out. The overall color profile suggests a population of evolved stars and low star formation activity. The lack of blue light indicates less recent formation of massive, short-lived stars.