The galaxy presents as a relatively smooth, elliptical structure. Its core is bright and concentrated, exhibiting a yellowish-white hue, possibly indicating an older stellar population. There is a gradual decrease in luminosity from the core outwards, suggesting a lack of significant ongoing star formation in the outer regions. The overall shape is closer to a sphere, with a slight deviation towards a more elongated form. There is no clear evidence of spiral arms or a distinct disk component. No signs of major mergers or tidal disturbances are immediately apparent, suggesting that if there was a past merging event it has since settled. The outer regions appear amorphous and unstructured, gradually fading into the background sky.
