The galaxy presents a predominantly smooth and rounded morphology. It exhibits a concentrated central bulge characterized by a yellow-orange hue, suggestive of an older stellar population. The surrounding galactic halo appears diffuse and fainter, displaying a gradual transition in color towards redder wavelengths with increasing distance from the center. There is a lack of discernible spiral arms or significant dust lanes, contributing to its smooth overall appearance. No signs of ongoing major merger activity or tidal distortions are evident. The integrated light suggests a system dominated by evolved stars with a relatively low star formation rate.
