The galaxy appears to be an elliptical type, with a generally smooth light distribution. The color gradient suggests a relatively old stellar population dominating the light output. The core is a bright yellowish orange, and the galaxy itself seems to possess an elliptical shape but is slightly elongated. There are no visible spiral arms or distinct dust lanes. The overall structure appears relatively undisturbed, indicating a lack of recent major merger events. There may be a faint diffuse halo surrounding the central region, but it is difficult to discern due to the limitations of the image resolution.
