The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core exhibits a bright, slightly yellowish hue, suggesting an older stellar population. The overall form appears to be relatively undisturbed, without significant tidal features or signs of a recent major merger event. The galaxy displays a radial color gradient, transitioning from the warmer central region to cooler, bluer outer regions. There is faint evidence of a disk or spiral structure, but the dominant impression is that of a spheroidal system. Based on the integrated light, the galaxy demonstrates moderate ongoing star formation activity. The overall roundness of the object indicates a probable E-type classification, although some disk-like structures cannot be ruled out.
