The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology with a high degree of roundness, showing minimal signs of disturbance or merging activity based on the surrounding structures. The galaxy presents a color profile indicative of an evolved stellar population, with a yellowish hue that suggests a population dominated by older, redder stars and minimal ongoing star formation. The galaxy appears relatively compact, with a concentrated light profile towards its center, further supporting the idea of a well-established and evolved system.