The galaxy presents a primarily smooth, elliptical morphology. The central bulge appears prominent and exhibits a concentrated, yellowish-orange hue, indicating a population of older stars. A fainter, more diffuse halo surrounds the central region, gradually fading into the background. There is some subtle evidence of an extended disk-like structure, but it is not sharply defined. It is difficult to discern significant spiral arm structure or dust lanes. There may be some minor disturbances, but no major distortions indicating significant ongoing merger activity are obvious. The overall shape is more rounded than cigar-shaped, suggesting it is closer to an E0-E3 type elliptical galaxy.
