The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The core region exhibits a reddish hue, potentially indicative of an older stellar population and/or dust obscuration. Moving outwards, the galaxy displays a gradual decrease in surface brightness, transitioning to a greenish-blue halo. This halo likely comprises a mix of older stars and a small number of younger, hotter stars resulting in moderate levels of star formation. There is a lack of distinct spiral arm structures or prominent dust lanes. Overall, the galaxy appears relatively undisturbed with no clear signs of major ongoing merger events or tidal interactions. The general shape is close to round, but not perfectly so, more between round and cigar-shaped. 
