The galaxy presents as a centrally concentrated, elliptical or spheroidal system. Its core exhibits a bright, yellowish-orange hue, suggesting an older stellar population. The overall morphology appears smooth with a gradual decline in luminosity moving outward from the center, showing no significant spiral arm structures or prominent dust lanes are visible. The galaxy is observed to be mostly symmetrical in shape. There is an indication of a faint halo surrounding the central region. The light is redder in the central parts of the galaxy. There are no signs of recent major merging activity.
