The galaxy presents as a flattened, elongated structure, suggesting a disk-like morphology viewed at a high inclination. The central region appears brighter and more concentrated, indicative of a bulge component. The color gradient transitions from a yellower hue in the central bulge region to bluer tints at the outer edges of the disk, which may signify younger star populations. There are subtle indications of faint, diffuse spiral arm structures extending from the central region, though these are not sharply defined. Overall, the galaxy exhibits a relatively smooth appearance, with no obvious signs of major mergers or tidal disturbances, though there may be minor asymmetries or perturbations hinting at past interactions. The absence of prominent dust lanes could imply a lower dust content, or alternatively, the high inclination could obscure any such features.
