The galaxy presents a generally smooth, elliptical morphology. Its overall color appears to be yellowish-orange, suggesting a dominant population of older stars and reduced ongoing star formation. The light distribution is relatively concentrated toward the center, lacking prominent spiral arms or disk-like features. There is no obvious visual indication of any major ongoing merger events or significant tidal disturbances. The shape is close to circular. The small degree of color variation may indicate subtle differences in stellar population across the galaxy.
