The observed galaxy presents as a relatively small, edge-on disk galaxy. The primary axis appears elongated and well-defined, indicative of a flattened morphology. A central bulge is visible, exhibiting a somewhat rounded but not perfectly spherical structure. Light distribution suggests ongoing star formation. The disk component shows a relatively smooth appearance, lacking prominent spiral arm structures. There is no obvious indication of major mergers or tidal disturbances. The overall color profile is dominated by redder hues in the central bulge, shifting towards bluer tones in the outer disk, potentially indicative of a radial gradient in stellar populations or dust extinction. The galaxy appears relatively isolated.
