The galaxy presents a generally smooth morphology with a high degree of central concentration. Its shape approximates a spheroid. There is no apparent disk structure or evidence of spiral arms. The color is primarily yellow/orange, suggesting an older stellar population and/or significant dust obscuration. There appears to be little ongoing star formation, consistent with its overall color. There are no obvious signs of recent or ongoing major merger activity. It could be a spheroidal galaxy, possibly an elliptical, and appears relatively undisturbed.
