The galaxy presents as a relatively smooth, elliptical-shaped object with a distinct central bulge. The core region exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the center, the color transitions to a slightly bluer tone in the outer regions, implying the presence of younger stars, although star formation appears subdued overall. There is no clear evidence of prominent spiral arms or a disk structure. The galaxy's shape is somewhat elongated, leaning towards an "in between" roundness, with a subtle cigar-like appearance. There are no obvious signs of major disturbances or ongoing mergers in this image; the overall structure appears relaxed and relatively undisturbed. The galaxy is well-defined with a sharp gradient between the central bulge and the outer regions. 
