The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a roughly symmetrical, diffuse light distribution. The core region is notably brighter than the outer regions, showing a gradual decrease in luminosity with increasing radial distance. The overall color appears to be towards the red end of the spectrum, suggesting an older stellar population. The galaxy shows minimal evidence of spiral arms or significant dust lanes. There is also little evidence of major merging events or tidal disturbances.
