The galaxy presents as a relatively smooth, centrally concentrated system. It appears to be an elliptical galaxy, exhibiting an overall elliptical morphology with a moderately high degree of central concentration. There is a slight elongation visible. The color is generally white, with subtle hints of blue towards the central region, and a slightly more orange hue surrounding the outer parts of the core. The light distribution suggests a general lack of distinct spiral arms or bar structures. There are no signs of active galactic nuclei or significant dust lanes apparent in the image, which contributes to its smooth appearance. There also does not seem to be any sort of tidal disturbance, implying that there have not been any major mergers. The image indicates a system dominated by an older stellar population, but some younger stars may exist in the central region of the galaxy, indicating a very low star formation rate.
