The galaxy presents an overall smooth morphology, suggesting it is likely an elliptical galaxy or a lenticular galaxy seen face-on. The light distribution is centrally concentrated, with a bright, yellowish core indicative of an older stellar population. The galaxy exhibits an elliptical shape. The color gradient transitions from a yellow/white hue in the central region to a bluish tint in the outer regions. This color difference may be due to a small amount of recent star formation in the outer regions. There are no discernible spiral arms or bar structures visible in this image. There is no evidence of any major merger events; however, there may be a small indication of minor disturbances in the form of some asymmetric distribution of light in the outer region.
