The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light profile exhibits a distinct nucleus, which is the brightest region. Moving outward from the nucleus, the light gradually diminishes. The overall color appears to be yellowish-orange, possibly indicating an older stellar population, as well as minimal recent star formation. There is no readily apparent spiral structure or distinct disk. There is a slight elongation or cigar shape to the galaxy. I find no obvious signs of tidal tails or major mergers, although very subtle disturbances cannot be ruled out at this resolution.
