The galaxy appears to be an elliptical galaxy with a relatively smooth, centrally concentrated light distribution. It displays a slightly oblate spheroidal shape. The core of the galaxy exhibits a yellowish-orange hue, indicative of an older stellar population and reduced star formation activity. Moving outward from the center, the color gradient transitions to a faint greenish color. There is no distinct spiral arm structure or prominent dust lanes visible. There is very little sign of an actively merging system. The galaxy's morphology suggests it is a mature system with a significant mass.
