The galaxy presents a generally smooth, elliptical morphology. Its light distribution is concentrated towards the center, with a gradual decrease in intensity towards the edges. It exhibits a yellowish hue in its central regions, suggestive of an older stellar population dominated by evolved stars. A subtle reddish tint appears on one side, possibly indicating a region of dust obscuration or a slightly younger stellar population contributing to the redder light. The overall shape suggests a relatively undisturbed system. The galaxy appears moderately massive, with a small amount of current star formation.
