The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge that appears a warm yellowish-orange hue, possibly indicating an older stellar population. Fainter and bluer outer regions suggest some ongoing star formation, although it is not immediately apparent as prominent spiral arms or distinct HII regions. The galaxy's roundness indicates it may be close to an E0 type elliptical. There is a faint hint of a disk but is not clear, with little evidence of major disturbances.
