The galaxy presents as a relatively smooth, elliptical-like structure. Its central region exhibits a bright, concentrated core that graduates outward into a less defined halo. The overall color profile appears consistent with an older stellar population, with the core exhibiting a yellow-white hue, transitioning to a redder color in the outer regions. There is no indication of prominent spiral arms or significant dust lanes. The shape is more rounded, with no apparent signs of major tidal disturbances or ongoing merging activity. Close inspection suggests no clear signs of active star formation regions.
