The galaxy presents as a centrally concentrated object with an overall elliptical morphology. It exhibits a bright, compact core that transitions smoothly into a more diffuse halo. There is some indication of minor asymmetry or disturbance in the outer regions, possibly due to tidal interactions or an ongoing merger. Faint, extended features emanate from the main body, potentially indicative of stellar streams or disrupted spiral arms. The color profile appears relatively uniform, with a slight bluing towards the outer edges, which may suggest the presence of younger stellar populations in these regions.
