The galaxy presents as a relatively smooth, elongated structure. The light distribution suggests an elliptical morphology, possibly of type S0 or early-type spiral viewed edge-on. A bulge is visible, appearing as a bright, concentrated region at the center. The galaxy exhibits a subtle color gradient, with the central bulge appearing more yellowish-white, indicative of an older stellar population. Fainter, bluish hues extend toward the outer edges of the disk, suggestive of younger stars and ongoing, though low-level, star formation activity. The disk component appears featureless, lacking prominent spiral arms. There are no obvious signs of major disturbances or ongoing mergers with other galaxies. The overall structure appears relatively undisturbed and relaxed.
