This galaxy presents as a centrally concentrated, smooth object with a notable lack of resolved spiral arms or significant dust lanes. The light profile suggests an elliptical morphology, or potentially a lenticular galaxy seen face-on, with a high degree of central symmetry. A slightly elongated shape is visible, but it is very close to being round. The galaxy exhibits a color gradient, appearing yellower at its core and becoming somewhat bluer towards its outer regions. This could be indicative of older stellar populations dominating the central bulge, with younger, bluer stars present in a surrounding disk component. There is no evidence of any on-going major mergers or tidal disturbances, though there may be minor signs of interaction in the form of faint irregular features or a slightly asymmetric halo.
