The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. There is a discernible central bulge, exhibiting a yellowish-orange hue, indicative of an older stellar population. Fainter, diffuse light extends outward from the core, with an overall elliptical shape. While generally smooth, some minor irregularities and faint blue tints hint at possible subtle disk-like features. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers, though some minor tidal disturbances might be present. There is not much in the way of substantial star formation.
