The galaxy presents as a somewhat elliptical, disk-like structure. Its core is visibly bright and concentrated, appearing yellow-white in color. The galaxy exhibits a relatively smooth texture across its observable body, with a subtle suggestion of spiral arms. The galaxy appears to be in a relatively quiescent state, exhibiting limited star formation. There is a subtle color gradient from the core outwards, with bluer hues towards the edges of the visible disk, suggesting a decrease in stellar age and potentially a low level of ongoing star formation in the outer regions. There are no signs of any major mergers occurring, but there is a potential for a very minor disturbance to the symmetry. The overall appearance suggests a galaxy that falls somewhere between a lenticular and early-type spiral, possibly transitioning towards a more passive evolutionary stage.
