The galaxy presents as an elliptical morphology, exhibiting a high degree of central concentration. The light distribution appears smooth, with no readily discernible spiral arm structure or prominent dust lanes. The central region is brighter and more reddish in color, transitioning to a more diffuse, greenish hue in the outer regions. The isophotes appear generally circular, suggesting minimal tidal disturbance or interaction with other galaxies. There may be a slight elongation of the galaxy along one axis, but overall the shape is close to circular. The color gradient from redder in the core to greener in the outskirts is consistent with an aging stellar population profile with potentially some ongoing star formation. There are no signs of recent or ongoing major merger events.
