The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears bright yellow, indicative of an older stellar population. The outer regions of the galaxy fade gradually into the background sky, with a redder hue appearing to be dispersed non-uniformly throughout the elliptical structure. There is no evident spiral arm structure or dust lane obscuration. Based on the apparent smoothness and lack of significant morphological disturbances, this galaxy does not appear to be undergoing a major merging event. The galaxy displays a high degree of central concentration with an apparently spheroidal shape.
