The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a dominant central bulge. There is little evidence of distinct spiral arms or significant dust lanes; the overall structure seems largely featureless. The galaxy displays a centrally concentrated luminosity profile that fades gradually towards the edges. A smooth transition in color from the core, which appears slightly redder, outwards is noticeable, indicating potential variations in stellar population and age. Faint outer regions of diffuse light suggest a stellar halo extending beyond the main body. No signs of tidal disturbances or ongoing major mergers are immediately apparent.
