The galaxy presents a flattened, elliptical morphology. The central bulge exhibits a concentrated, bright yellowish-white hue, suggesting a population of older stars. Extending outward from the bulge, a fainter, somewhat bluer disk is observed, indicating the presence of younger stars and ongoing star formation. The disk appears relatively smooth with no obvious spiral arm structures. The overall shape is elongated, leaning toward a cigar-like appearance. There is no significant evidence of major disturbances or mergers. Minor asymmetries or disturbances in the outer regions of the disk may be present, but are not definitively discernible given image quality.
