The galaxy appears to be a relatively small, edge-on or highly inclined disk galaxy. It exhibits a flattened, elongated shape with a smooth, diffuse light distribution across its body, suggesting a relatively featureless structure. The central region appears slightly brighter and potentially more concentrated, but there is no evidence of a prominent bulge or a well-defined spiral arm structure within the visible wavelengths. The color profile indicates a reddish hue, possibly indicative of an older stellar population or the presence of dust obscuring bluer light from younger stars. The galaxy's dimensions suggest a compact size, and there are no visible signs of any major mergers or tidal interactions distorting its overall morphology.
